SUBJECT AND OBJECT INDEX

Accretiona-model for Keplerian disk flows, 399,401-404~-model , 404beat frequency model, 446-447,465-468. 477-478beat frequency modulated, 365-366bundIe, 412by aligned rotators. 401, 407, 410by oblique rotators. 401capture radius, 366. 369-372. 391central corona. 455, 459. 463. 467. 471Comptonized bremsstrahlung models. 404,414disk. 139. 249, 251, 254-255. 289.293-294. 296-300. 304-3OS, 307. 309,311. 446. 453-454. 459-461, 493-496,503-504. 506-507, 509-510disk corona. 302, 3OS. 310disk instabilities. 139. 501. 50s,509-513disk thermal time, 509disk viscous time, 506-507Eddington-limited, 222-223. 228. 497exterior flow, 366-376. 381flows. 493from a Keplerian disk. 366-367.375-379, 381-382. 384-390. 397-401,410. 412-413. 415. 418. 420. 424funnel, 431gas-pressure-dominated region, 399.403-4OS. 413-414induced collapse. 81. 103-104. 110.112-113, 119-121, 143. 146-147.153-159. 167. 261, 341inner disk corona. 445-447. 455-456.459. 471, 475

---, luminosity. 367-368, 535. 539---, mass. 225

numerical simulations. 372-374on a white dwarf. 103-1OSonto compact objects. 245, 251. 253radial flow. 375-376. 378-382. 390-397.400. 445-447. 456. 459-460. 463. 471,475. 477radiation-pressure-dominated region. 399.403-4OS. 414

579

radius, 494, 526spin-down torque. 418-420. 423spin-up torque. 418-420, 423stream. 302strong interaction region, 399supercritical. 297torques. 254. 414-425rwo-temperature disk models, 404. 414via stellar wind, 254-255. 292. 494

Alfvenradius, 384, 393, 397-398, 413

---. velocity, 239, 383-384---. wave. 85. 383. 393, 521-523Angular momentum

captured, 494-495---. loss. 111-112, 161, 184. 186-189. 197.

199.496Annihilation

affected by magnetic field. 562electron-positron, 191. 561-563. 568radiation, 561. 568rates, 562redshifted lines. 561spectra, 563-565

Atoll sources. 260. 319-320. 322-323.326-328. 334. 337-338. 478high frequency noise, 334power spectra of. 332-334

Be stars. 493. 501---. wind from. 493Beaming factor. 109Binary system(s)

accreting. 225, 227Be-neutron star, 499detachment. 112eccentric orbit. 293. 296-297eclipsing. 572

---, equipotential surface. 290-293evolution. 230. 374evolved companion, 495high-mass, 363-364. 366. 369, 373-374interacting. 159-160. 219, 224low-mass. 363-365. 367. 369. 374.413neutron star, 445-478neutron star-white dwarf, 117, 495orbital period, 245. 376

580

Black hole candidates. 245-246. 296. 299. 308.364. 478. 501-503. 509. 548

Bowen mechanism. 298Bragg reflection. 485-486Bubbles. expanding. 107

Carbon-'-. burning front. 149---. deflagratlon. 105. 149-151. 156Cataclysmic variables. 197-200. 203. 25 1. 312.

494. 504. 508. 510. 577binaries. 186-188magnetic. 250non-magnetic. 250orbital period distribution. 252period gap. 187-190statistics. 261

Cerenkov---. atmospheric technique. 571---. showers. 571Chandrasekhar mass. 147. 153. 158Chapman-Ferraro radius. 394. 397. 400Chemical separation. 153Circulation currents. meridional. 292Close binaries. 164. 368-369

evolution of. 109. 171.... high-mass system. 493"-. low·mass system. 493Coherent flow. 49Collapse

accretion-Induced. 81, 103-104. 110.112-113. 119-121. 143. 146-147.153-159. 167. 261. 341core. 143-144electron capture induced. 156-157iron core. 143. 161

Colour indexB-V. 249. 300. 305

'--. opticaJlX-ray. 249---. U-B. 249. 300. 305Common envelope. 147-". evolution. 161Companion winds. 203-204. 211. 216Companion evaporation. 171, 180. 190. 193---. model of. 190-191---. timescale. 191Compton

cooling. 391, 393-394. 404. 473. 518.552heating. 552scattering. 335. 470. 485. 488

Conductivity---. electrical. 71. 235-241. 378-379. 406.

408. 412. 419---. thermal. 89. 236. 293Convection. 520-521Convective equllibIium. 292Cooling---. bremsstrahlung. 391, 393. 404. 463-464

Compton. 391. 393-394. 404. 473. 518.552cyclotron. 391. 562via electron-ion energy exchange. 391.393X-ray. 393

Cooper pairs. 49Core width to peIiod relation. see pulsar radiationCorona. 496---. scattering. 496Coupling time---. crust-core. 65---. crust-superfluid. 60Coupling. superfluid and crust, 52. 54Crab nebula-". pUlsed radiation. 571-572. 576-'-. unpulsed emission. 571-572Crust

bremsstrahlung, 93crust·core coupling. 44Inner. 34. 47. 90lattice nuclei. 37neutron superfluid. 57-58of neutron star, 58-62outer. 88pinning to the lattice. 54spin-down. 52-53.92

Crustal superfluid. 58.59.67---. coupling time. 60---. pinned. 60.64.67Crystal lattice, 53Cycle'-'. CNO 518. 520, 532. 539. 541---. pop. 518. 537Cyclotron

absorption. 224, 488-489cooling. 391. 562emission. 376. 382. 435. 455. 461. 488energy. 490excitation. 487-488fearures. 5 ISharmonics. 484. 489lines. 253-254. 545-559. 561

radiation. 568resonant scanerlng. 545. 550-556

---. scattering lines. 365. 376

Dark cloud, L1457. 517Delayed detonation. ISO-lSi. 153Detector deadtime. 320. 329Diamagnetic disk model, 385-387DUfusion---. laminar viscous. 50---, viscous time. 50Dipping. 496Dispersion measure. change in. 50

Eddingtonlimit. 296-297. 332. 339-340

---. luminosity. 401. 445-447. 454-455. 458.460. 471. 532. 539. 541

Ekman pumps. 50Electron---. capture.. 152-154, 156. 518---. conduction. 520Emission---. lines, 153---. non-thermal radio. 297Energy dissipation. thiOUgh vortex line creep. 59Envelope---. common. 181-182---. hydrogen rich. 184Explosive I

burning front. 154---, oxygen bUrning, 154 ,

Flashhelium. 158, 520. 532. 535-537.542-543hydrogen. 158. 519-520. 532, 535.542-543thermonuclear model. 531-544

Foller-Planck approximation. 432-433, 435

Gamma ray(s)emission; 571-572observations. 571. 576Observatory. 425PeV emission. 426production. 376. 406. 425. 428. 430sources. 72. 84. 363. 394

---. TeV emission. 426-427very high energy. 571

Gamma ray bursters. 224. 364. 483. 489-490

581

Gamma ray bursts. 71. 84-85. 192. 515. 524.526. 561-568energy dips. 546. 550. 553GB 720514. 548GB 780325. 546. 549

---. GB 781119. 547GB 790305. 85GB 790412. 546. 549GB 790612. 546. 549GB 790731. 548GB 820125. 548GB 821016. 548GB 870303. 545. 553GB 880205. 489. 545. 550. 556-558GB 890929. 545, 553rapid variability. 546

Geomagnetosphere. comparison with neutron starmagnetosphere. 380-382Globular cluster(s). 222, 232. 338. 341. 509

binary formation in. 114---. Terzan 5. 112. 180. 191. 214. 216-217---. M15. 202,342Gravitational

radiation. 112. 184. 186. 188-189. 197.199, 496settling of elements. 518

Hartree-Fock approximation, 13. 16. 128-129---. free energy per nucleon. 128-129Hartree-Fock-Bogoliubov approximation. 8Helium stars. 143. 146. 159-160. 163-164.

166-168. 184---. exploding models. 162. 164-165

Instabilityaccretion-line. 374convective. 149current-driven. 428disk. 501. 505. 509-513dwarf-nova type, 511illumination, 501. 505-509

---. Kel"tn-Helmholtz, 385, 387-388.393-396. 419mass transfer. 504-506. 513Rayleigh-Taylor. 159. 162-163. 393-396thermal. 504, 509

Intermediate polar. 517Interstellar---. absorption. 324---. medipm. 524-526Ionizing radius. 526

582

Kick velocities. 165-166

Lagrangean point. 290-291. 5OS-507. 572Landau---, levels. 487. 522, 552. 554---. orbitals. 484Light curves

ellipsoidal, 289, 291-293---, ellipsoidal variations. 290-293---. optical. 289-313Luminosity

critical. 459Eddington. 401. 445-447. 454455, 458.460. 471. 532. 539. 541X-ray. 445-481

Magnetic axis---. allignment of. 357---. inclination angle of, 356-361Magnetic braking. 112. 184. 186-189, 197.

199. 340-341, 374, 50sMagnetic diffusivity, 379. 385Magnetic dipoles---. perpendicuiar. 80-81---, spin aligned, 80. 82Magnetic fieid

decay of, 90. 92decay timescale, 230expulsion, 226-227. 232. 240London fieid, 51-52opacity dependence on, 88reconnection, 225. 385. 387-389. 395.410. 412. 418, 428. 430, 522residual, 222-224, 227, 232

Magnetized scattering atmosphere. 485Magnetopause. 392-393---, stabie. 393. 395---. unstable. 393. 395-396Magnetospheric flow. 382-384---, stable. 397-398Magnetostatic boundary, 111Magnus---, equation, 52---, force, 59-60Many-body formalism

correlations. 42direct interaction. 41-43Fermi liquid model. 39long range correlation. 39

---, quasiparticle interaction. 46RPA equation. 39

Mass transfer. 104. 110. 116. 180-182.184-189. 191, 197-202. 494. 496-497in evolution of close binary. 146

---. mechanisms. 368-375rapid rotation. 247

---. via stellar wind, 146. 158-159. 247. 254Matter---, pion condensed, 21, 27-30. 34---. quark. 21, 30-31, 33---, strange quark, 21, 31-33---. strangeness condensed, 21. 29-30Matter at subnuclear densities

Coulomb energy reduction, 3. 12-13.16-17electronic properties. 3-5non-spherical nuclei. 3. 13, 16-18surface tension of nuclei. 3. 9. 12-13. 16.18thermal energy. 15

Molecular cloud, MBM 12.517

Nebula(e)Crab. 104. 107

---. planetary, 111synchrotron (plerion). 107-108X-ray synchrotron, lOS

Neutrinobremsstrahlung, 37. 89. 91cooling. 88-94emission, 27. 37. 87-88. 93flux. 132heating. 126modified Urca process. 37. 89transport, 14. 125-126. 130. 133.136-137

Neutron drip. 4. 8-11. 13. 18. 33Neutron matter. 58-59. 67---. equation of state. 58. 67Neutron pairs, 51Neutron stares)

accretion, 319. 336. 338-340, 363-439.493.502, 516-517. 524. 526. 531-532.535-538. 542-543, 573accretion disk. 483. 486aligned, 259atmosphere. 88BlBe companion. 230. 232binding energy. 125. 138black body radius. 256centrifugal radius. 397cooling. 37. 94, 239

core. 53. 90. 235-241corona, 502austal density. 58densities. 3eclipslog companion. 427

---. equation of state. 22. 25. 30. 33-34.88-89. 91. 93. 95flarlog. 425

---. formation. 103-104. 113-120. 125. 143.261formation rate. 106gatnrna ray emission. 571graveyard, 178-179. 192heat capacity. 93in binary systems. 114-115. 131. 227.366-367. 379in eyg X-3. 33in PSR 1913+16, 34in SN 1987A. 25-26. 33in X-ray binaries. 245-277inner crust. 53low-mass binary. 483magnetized, 246. 253magnetopause. 392magnetosphere, 249. 332. 340, 363.365-366. 368. 375-400. 405-410.445-446. 453-455. 460-461. 466-467.475. 477. 495magnetosllheric radius. 516mass-radius relation. 58. 257masses of, 24orbital velocity. 368. 370particle acceleration in magnetosphere.424-430plasma capture from companion. 366.368-375plate tectonics. 71-85population of. 104progenitors. 109. 110propellor braking. 341proton fraction. 10quantum liquid core. 58radiation from. 204. 212rapidly rotating. 33-34recycled, 171, 181, 192-193reheating. 91-93rotation rate, 339rotational evolution of. 3runaway. 181slowly accreting. 515. 517-518. 524

_... spin·down. 75. 79-80. 85. 200. 227.341, 421

..•. spin history. 54spin frequencies. 365. 420-421. 426spin-up. 75. 79-80. 82. 252. 407. 416.421. 495statistics, 484strange star. 22-24

---. temperature. 3thermonuclear flash. 338wind from. 532

Neutron star crust. 21. 24. 32-33, 58-62. 88.90.254cracking. 71. 74-77. 84-85lattice yield, 76melting temperature. 72plastic flow in. 73. 83plate motion. 77-78properties. 72-74shear stresses on. 74-75. 79spin-down. 71. 76-77spin-up. 71. 76-77

Neutron star magnetic field, 245. 320. 332.339-342. 445-446. 493. 515. 518. 523decay. 54, 171, 175. 192-193.219-232.261decay timescale. 556evolution. 3. 37. 79, 81. 174. 219-232.235-241history. 261interacting with accreting plasma, 366.375-400. 406-410. 416. 418. 425. 429

---. orientation, 546. 554strength. 219. 247. 253. 259. 261. 319.364-365. 379. 427. 431. 446. 453. 466.478. 545-546, 550. 552, 555-556. 558stresses. 71. 74-75

Neutron star matter. 37-47equation of state, 88-89. 91. 93. 95exotic matter. 92-95in liquid interior. 21pion coodensates, 91, 95

Neutron star <\Iurfacehelium fueld, 538hydrogen fuel. 538ignition, 538. 541nuclear fuel. 538-539

Noise, 329-336. 338high frequency. 327-329, 331-336.340-341. 450

583

584

low frequency. 329-332. 334-335.450-451. 466. 468469Poisson. 329very low frequency. 328-332. 334-335.450. 466, 468white, 329

Nova(e)dwarf. 139.304.504,509-510.512

---, explosion. 104, 147. 158---. optical. 311Nuclear

equation of state. 22. 25. 30. 33-34---. liquid-drop model, 3. 6-9, 13---. partition function. 127Nuclear burning

behavior of, 531---. global analysis, 535-539---. stability of, 531. 538-539. 542Nucleon effective mass. 54Nucleosynthesls. 161-163---. explosive, 160

Ohmic dissipation. 219. 235, 239-240Optical thickness. Thompson. 487Overflowing---, atmosphere. 368-369. 374-376---. envelope, 368-369, 374-376Oxygen deflagration. 156

P-Cygni profiles. 153Pairing (see also superfluidity)

gaps. 37-38. 4346---. interaction. 38-39. 43-46

matrix element, 38-39S-wave pairing, 37-39

Particle beamingemission height. 355geometry of. 351-352. 355high y. 349. 359. 362low y. 349. 359. 361

Phonons. 55Photometry. CCD. 309Plasma diffusion, onto magnetic field lines, 395,

401. 410Polarimeter

photoelectric. 485---. spectral X-ray, 486---. X-ray. 485Polarization---. degree of. 562-563. 567

measurements. 568Propeller mechanism. 516Proto-neutron star. 135Proton

decelaration at stellar surface. 430438flux lines. 54flux tubes. 226-227supercondueting, 226

Pulsar(s)acceleration potential. 353-354accretion-powered, 363-366. 379. 383.394, 396-397. 403. 406, 408. 413414.423-427. 435, 467468. 483. 487.490-491, 556alignment. 82apparent age, 96binary. 103. 116. U8. 166-167. 222.230binary millisecond. 143binary radio. 171-173. 177-179.181-182. 184-186. 193birthrate. 109. 120companion evaporation. 82. 117.119-120. 197. 200-201conal emission. 349-362cooling. 87-99core emission. 349-362crust motion. 82-84death line. 85. 119, 172, 178-179. 192,222-223. 228-230dispersion measure, 232eclipsing binary, 180. 191, 213-214, 216emission geometry. 349-362equilibrium spin period, 176

---. exponential decay of magnetic field, 515exponential relaxation, 55glitches. 37. 49-51. 57-59. 62-67. 71.82-84graveyard, 222-223hollow-cone beam, 349, 351Hubble line. 118-119, 172. 178-179. 223in globular clusters, 103, 113-120. 173kinetic age, 220-221. 225low-mass binary. 146.159magnetic field, 118. 171-172.214-215.515magnetic field strength. 107-108millisecond, 71. 75. 77-78. 80-82.171-174, 180-181, 190, 192-193.197-204. 212-213. 216. 218. 223-224.252. 261. 365. 466. 477. 572

origin of binary. 164-167---. pencil beam. 349

polar cap. 349, 355. 359population. 109post-glitch behavior. 45. 47. 59. 62-67post-glitch relaxation. 51, 54-55PSR 0021-72A, 119PSR 0021-72C, 173PSR 0021-720, 173PSR 0021-72E, 173PSR oo21-72F, 173PSR 0021-72G. 173PSR 0021-72H. 173PSR 0021-721. 173PSR 0021-721. 173PSR 0021-72K. 173PSR 0021-72L, 173PSR 0031-07. 96-97PSR 0355+54. 97. 573PSR 0531+21 (Crab). 50-51. 55. 57, 62.64-67, 71. 82-83, 88, 96. 190. 358,426, 548. 571-573PSR 0540-69, 83,96PSR 0655+64. Ill. 173. 177-178, 181.192. 222. 224, 261PSR 0656+14. 96-98PSR 0820+02. 112. 173, 177. 186PSR 0823+26. 357PSR 0833-45 (Vela). 50-53. 57. 62.65-67. 71. 82-83, ~5. 96-98. 357PSR 0906-49, 358PSR 0950+08. 96-97PSR 1055-52, 96-97. 358PSR 1257+12, 173PSR 1310+18, 173PSR 1509-58, 83. 96, 572-573PSR 1516+02A. 173PSR 1516+02B. 173PSR 1534+12, 111, 165-167. 173, 177

---. PSR 1620-26, 173, 177. 186PSR 1639+36A. 173PSR 1639+36B. 173PSR 1642-03, 96PSR 1702-19. 357PSR 1737-30. 50. 83PSR 1744-24A, 110. 119, 173. 180.201. 203. 213-218PSR 1746-20. 173PSR 1800.83PSR 1802-07, 173PSR 1818-04. 358

PSR 1820-11. 173. 179PSR 1820-30A. 173PSR 1820-30B. 173PSR 1821-24. 82. 173. 572-573

---. PSR 1822-09. 358PSR 1823. 83PSR 1831-00. 173. 177PSR 1855+09. 81. 112. 120. 173. 177.224. 572-573PSR 1908+00. 173PSR 1913+16. 34. 111. 165-167. 171,173, 177-178. 186. 193.254.261PSR 1929+10, 96. 98. 357PSR 1937+21, 81, 96-97, 112. 173.180. 190. 203. 214. 572-573PSR 1951+32. 96PSR 1953+29,82. 171. 177-178. 185.193. 357. 572-573PSR 1957+12. 112PSR 1957+20. 81. 112. 118-119. 173.180. 191. 200. 203-204. 213. 216-218.572-573PSR 2127+11A, 173PSR 2127+11B, 173PSR 2127+11C, 173PSR 2127+110. 173PSR 2127+11E. 173PSR 2303+46. 111. 173. 177. 192radiation-powered, 365radio. 104. 106. 108. 111-121. 203.212. 222, 232. 571-573. 576recycled, 111, 113. 171. 178-180. 192.197. 223. 225. 227. 230-232. 414reheating. 93rotation-powered, 425-426. 466. 548.556runaway. 182spill periods. 76spin-down. 57. 59, 61. 64-65. 77-80.82-84. 172. 178, 226-227, 230. 232.516. 556

---. spin-down age. 220-221. 225. 228.353-354 I

spin-down luminosity. 118spin-down rates. 49-50. 52spin-up. 77-79. 115. 119. 176, 178.180. 192-193. 222. 224. 254

---. spin-up line. 82. 118. 172. 177-179.222-223. 228. 230. 414starquakes. 57-67

585

586

. statistics. 106. 171. 197-202. 224.572-576

---. superfluidity. 57-67---. timing noise. 50

transient. 424---, turnoff. 84

velocity, 220white dwarf companion. 222. 224wind, 112, 115-116. 197. 200wind driven X-ray. 574X-ray. 84. 174. 255. 363. 571. 573-576z-distrlbution, 220

Pulsar magnetospheredipolar structure. 362

---, open field lines. 349. 357---, velocity of light cylinder. 355Pulsar radiation. 349-362. 571

circular polarization. 350. 353. 359core-width to period relation. 355-357.360-361curvature radiation. 359Interpulsars. 354. 356Interpulse profiles. 354-355linear polarization. 350, 353. 359-360.362polarization. 350pulse profile classification. 349-360pUlse profiles, 354quasi periodic modulation In polarization.353spectral evolution of. 350

Pycnonuclear reaction. 154

Quantized magnetic flux lines. 52Quasars. 245Quasi-periodic oscillations. 247. 259·260. 308.

319-320. 324. 329-336, 338-341,445-478. 486, 493. 498flaring branch, 331-333. 335. 339. 342.449. 451-453. 460. 476-477frequency. 331, 335horizontal branch, 330-333. 335, 337.339, 341-342. 364-366. 414. 449-453.460, 465-469. 477magnetospheric origin. 330. 337, 339-340normal branch. 330-333. 335. 339. 342.449. 451-453. 460. 469-477

Radiationcurvature. 484

---, gravitational. 340-341, 368. 374. 505

synchrotron. 484Radioactive decay. 151, 164. 168---. light curve. 151Relativistic motion. see particle beamingResistivity

electrical. 235-236. 238-239Hall. 236-238

---. longitudinal. 237-238trasverse. 237-238

Roche lobe, 159. 165. 290detachment from. 188-189

---, filling. 183-184. 187. 189. 197-199.495. 503filling companion. 119. 517

---. filling primary. 247. 291overflow. 147. 149. 161, 166. 178.180-182. 247. 249. 293. 305. 486.493-494radius. 200shrink. 180underfllling. 198-199underfllling primary. 247

Roche potential, 507Rosseland absorption coefficient. 292

SatellitesAriel-5. 259-260. 339EXOSAT. 87-88, 96-98. 254. 256. 305.319-320. 322-324. 326-329. 338. 424.445Glnga, 230. 312. 326. 445, 545.550-551. 556-558Hakucho. 326. 445HEAO-l, 259-260. 546. 550OSO 8.445ROSAT, 87-88. 96. 98-99. 499. 526SAS-3, 257. 532Spektrum. 485Tenma, 328. 445UHURU. 87.246Venera 11-14, 546

ScatteringCompton. 470. 485. 488Inverse Compton. 335Raman. 553-556resonant. 522stimulated one-photon. 491two-photon. 487-489. 491

Schwarzschild radius, 563Sonic point, 210---. In radial flow. 204-206

with heating. 207-208Sources

GK Per. 517---. GT 0236+610. 297

H0253+193.517-518Sk-69~02. 138

Spectral index---. gamma ray. 546---. X-ray. 546Spectrographs. ceo. 254Spectrum

emission lines. 249. 251---. variable emission/absorption components.

247Starquakes

elastic energy in. 51---. model. 51---. on neutron stars. 57-67Stars

Be. 247.249HO 226868, 245HO 77581. 248HZ Her. 312x Ori. 248K rype. 311K3-7 dwarl. 31novae type. 245° rype giant. 246tidal deformation of. 114U Gem rype. 245

Statistical---, absolute rms variation. 336---. fractional rms variation. 329Stellar

core collapse. 125. 127. 130. 136.138-139energy transpon in core. 3model. 125numerical simulation of collapse. 125-126.130, 138

Stellar windradiation-pressure-driven. 368-369, 374.405self-excited, 368-369thermally-driven, 372

Stokes parameters, 562Superconductivity. 49---. in protons, 37-47. 58. 75Superfluid

dynamical coupling time. 53-54---. dynamics. 49. 51-53

energy gaps. 49. 51. 58-59. 67. 75-76in core. 53-54in crust. 53-55. 57-59. 67instability of. 50-51neutrons. 37-47. 51-53. 57-59. 71-72.74-77, 90. 92. 226. 237-238pinned neutron. 60. 64. 67protons. 51-53quantized vortices. 51-52transition. 72transition temperarure. 58-59vonex pinning. 59

Superfluidity • 49-50. 93Superfluidity in neutrons 37-47. 51-53. 57-59.

71-72. 74-77, 90. 92. 226. 237-238BCS theory. 37, 43. ~5

BCS week coupling, 38coherence length. 37pairing. 37-47

Supergiant(s)---, B,493---. 0,493Supemova(e)

assymetries. 110dumpiness, 163delayed explosion. 133. 135energy in explosion. 125. 134, 136explosion, 105. 110. 120

---. explosion mechanism. 136from core collapse. 125. 136"hot bubble" explosion, 135hydrogen-rich envelope. 146Kepler's. 104light curves. 164mass ejection. 166model. 125-126. 132-136neutrino-driven. 131numerical simulations of, 125-126. 130.134silent. 104SN 1572. lOSSN 1604. 105SN 1972E. 152-153. 164SN 1981B. 152-153. 164SN 19831, 164SN 1983N. 152. 164SN 1987A. 25-26. 33, 132. 134-136.138-139, 144. 151SN 1987K. 105. 145-146SN 1987L. 144-145SN 1987M. 144-145. 152. 164

587

588

---. SN 1987N. 144SN 1989B. 153SN 1990N. 151spectra of. 144spectroscopic classification. 143

---. Tycho·s. 104---. type I. 104. 143

type Ia. 104. 149-153. 156. 158type Ib/lc. 104. 143. 164-167type II. 104

Supernova remnants. 103. 106-109. 222---. hollow shell. 107---. plerionlc. 107Synchrotron radiation. 85. 523

ThennonucIearburning. 531-544burning front. 132flash. 256. 258-259. 365flash model. 531-544model. 524runaway. 515. 518

Thome-Zytkow star. 181-182Tidal---. capture. 114-115. 117---. interaction. 376Transition temperature. 49Transport coefficients. 235-236Turbulent diffusion. 387-389

Ultrarelativlstic heavy ion colIislons. 34-35

Vortex line(s). 37. 43. 52-53. 74-75. 77,226-227creep. 58-61. 92creep model. 50. 54-55creep theory. 60-61. 63. 67density of. 63energy gap. 49motion of. 52. 60. 63. 227neutron. 54. 226-227. 232of supertluid neutrons. 89. 92-93pinning. 37. 45. 58-59. 71-72. 74-77.82-84. 92. 226-227pinning energy. 54. 59. 61-63. 67. 76.227pinning force. 59. 75. 78. 227replnnlng. 64. 67scattering. 55strong pinning. 61-62superweek pinning. 62-65

unpinning. 37. 50-51. 55. 64. 67. 75-77,82week pinning. 62-64

Wave(s)Alfven. 85. 383. 393. 521-523conductive carbon deflagratlon, 155-156convective deflagration. 149. 153detonation. 149. 154gravitational. 136shock. 132-134. 204. 370. 392-394.425. 431, 520. 524-525

White dwaIf(s). 81-82. 103. 111. 143. 146.153. 423-424. 504. 508accreting. 143. 147-149. 158C+O pair of. 147carbon and oxygen. 147. 153-155. 157collapse of. 153-156disruption. 151. 156double system. 147. 166expansion of. 151explosion. 154-156heat wave in. 149hydrogen shell burning. 147-148interior temperature. 147thennal runaway. 154

Winger-Seitz approximation. 11WOlf-Rayet stars. 146. 159. 163-164

X-ray(s)albedo. 292antapex. 325-326. 331-332. 340apex. 325. 330-331. 340banana states. 260. 327-328. 332-334.337. 342colour. 320. 323. 326. 334colour-colour diagrams. 260. 320-329.338. 342. 445-446. 448-449. 462. 478Compton scattering. 427cooling. 393counting statistics. 329dips. 298-300. 302. 304. 338. 341-342.497-498eclipses. 298. 300. 302. 307flares. 309. 365. 394flaring spectral branch. 325-326. 330-332.334. 337. 340. 445-450. 452-453.464-465hard, 393hard colour. 323. 325. 327

hardness-Intensity diagrams. 259. 320-328.324. 338. 342. 445-446. 448. 462. 465.478hardness of spectrUm. 501hardness ratio. 320-322. 324heating. 289. 293-294. 296. 298. 300.304. 310-311horizontal spectral branch. 325-326. 328.330. 332. 337. 340. 445-450. 452-453.460-462illumination. 496-497. 511island states. 260. 327-328. 332-333. 342light curves. 494. 502. 506. 508

---. millisecond pulsars. 342normal spectral branch. 322. 325-326.328. 330-332. 334. 337. 340. 445-450.452-453. 462-464oscillation frequency. 414outbursts. 296. 311-312period modulation. 496photospheric radius. 532polarimeters. 485 -486polarized emission. 483. 486power spectra, 325-326. 329-334. 424.446. 449. 450-453pulsations. 253-254. 259rapid variability. 320. 324-326. 329.334-336. 338. 342

---. recurrent outbursts. 297. 310reprocessing. 289. 298soft. 368soft colour. 323. 325. 327spectra. 259-260. 289. 308. 320.334-336. 338. 430. 445. 478. 502spectral hardness. 259spectral Index. 546synchrotron. 215thermal emission. 87-99thermonuclear flash. 174-175time lag. 334-336two-component spectral model, 336Variability. 289. 308Z-shaped spectral pattern. 445-446.448-449. 462. 478

X-ray binaries. 110-111. 166Be. 166. 247. 249. 253. 297. 495bootstrapped evolution. 212-213. 217

---. classification. 319. 338-342companion evaporation. 146. 218. 252components In conjuction. 289

---. degenerate dwarf companion. 340

589

distonion of companion. 289eclipsing. 293. 296. 299. 503ellipsoidal brighmess variations. 297-299.305. 311-312

---. evolution. 181-191. 319. 338. 340-342.493.508evolved companion. 340-342. 508-509galactic distribution of. 253high-mass. 110. 171-172. 174-175.180-193. 245-277. 287-297. 493-495.501low-mass. 78. 80-82. 110-113. 115-116.120. 143. 146. 156. 197-203. 209. 211.224. 245-277. 298-313. 319. 322-326.329. 336-337. 445. 478. 486. 493-498.501. 508. 510-511main sequence companion. 340neutron stars In. 245 -277nuclear evolution of secondary. 505optical brightness variations. 296-297. 300.302. 304-305. 308optical light curves. 289-313orbital Inclination. 299. 302. 307-310.447orbital period gap. 200orbital periods. 183. 249. 251-252. 289.293. 296-297. 300. 303-305. 307. 309.311. 338. 340-342. 447. 503. 508-509orbital variations. 289. 293. 296panial eclipses. 300populations. 319radiation driven evolution. 197-202recurring eclipses. 300spin-down. 212spin-up. 203. 216statistics. 197. 201. 212superior conjuction. 293. 296. 300. 302tidal distonion. 289two-temperature Inner disk. 509very low mass. 211Z-class. 451-453. 460-461. 469. 475.477-478

X-ray burst(s). 174-175. 255-259. 298. 300.311. 319. 322. 337-339. 341. 365. 447.501-503.510.524.531-544cooling track. 337duration of. 337-338In globular clusters. 532luminosity. 535profiles. 532. 533. 534spectra. 534

590

---, type I, 255-256, 260---, type II, 255, 257X-ray burst sources, 247. 251. 256. 259. 261,

309, 338, 341-342, 486487, 5314U/MXB 1636-53, 5334U/MXB 173544,533,5434U/MXB 1820-30, 5334U/XB 1608-52. 533, 543

---, Aql X-I, 553, 543Cen X4. 533GX 3+1, 533MXB 051240, 533MXB 0748-67, 543MXB 1659-29, 533, 543MXB 1724-30,534MXB 1728-34, 533-534MXB 1730-335 (Rapid Burster), 533MXB 1743-29, 534MXB 1837+05 (Ser X-i), 533,543MXB 1850-08, 534MXB 1906+00, 533MXB 1916-05, 533XB 1745-24, 533

X-ray observatoriesAXAF.99

---, EINSTEIN. 87-88, 96-98---, Imaging X-ray telescopes, 88,94X-ray sources, 363, 382, 393-395, 424

0050-727 (SMC X-3), 2710053+604, 2710053-739 (SMC X-2), 2710103-762, 2710114+650, 2710115+634, 175, 271, 573-5740115-737 (SMC X-I), 175-176,254-255, 271. 293-294, 5740236+61, 2720331+530,272,5740352+309, 272, 5740512-401, 262, 5330521-720 (LMC X-2), 183, 262, 4470532-664 (LMC X-4), 176, 254, 272,295-296, 5740535+26, 176, 272, 5740535-668, 272

---, 0538-66 (LMC X-3), 272, 295, 296,5740540-697 (LMC X-I), 272, 5480543-682 (CAL 83), 183, 262, 3070544-665, 2730547-711 (CAL 87), 183. 262, 299

---, 0556+286, 2730614-H>91, 2620620-003 (V616 Mon), 183, 262,311-312, 501-504, 509, 511-5120726-260, 2730739-529, 273

---, 0748-676, 183, 198, 201-202, 257.262, 3~301, 503, 5430749-600. 2730900403 (Vela X-I), 24, 34, 53. 175,248, 254-255, 273, 293-294, 374. 427.548, 571-5750918-549, 2630921-630, 183, 263, 300, 3421024.0-5732, 2731034-56, 2731118-615, 2731119-603 (Cen X-3), 176, 245-246,254, 274, 293-294, 364, 423, 573-5741145-619, 255, 5741145.1-6141, 2741223-624 (GX 301-2), 175, 274,296-297, 3741249-637, 2741253-761, 2741254-690, 183, 263, 300, 3021255-567, 2741258-613 (GX 304-l), 2741323-619, 183, 2631354-64 (Cen X-2), 2631417-624, 275.5741455-314 (Cen X-4), 183, 263,311-312.502-503,508-509,511. 5331516-569 (Cir X-I), 246, 263, 342, 4781524-617 (TrA X-I), 2631538-522, 175, 254, 275, 3741543-475, 2641543-624, 2631553-542, 2751555-552, 2751556-605, 2641608-52, 264, 326, 328, 533, 5431617-155 (Sco X-I), 87, 175, 183,245-246, 250, 264, 307, 311, 323-326,331-332, 334, 337-340, 445, 447,449-453, 464-465, 477

---, 1624490, 183, 264, 342---. 1626-67, 176, 224-225, 574

1627-673, 175, 183, 259, 2641630472, 264, 501-503

---. 1636-536. 183. 264. 308. 322. 324.326-328. 333. 338-339. 5331642-455 (GX 340+0). 265. 325-326.330. 332. 334. 339. 4531656+354 (Her X-I). 53. 175. 183. 192.209. 211-212. 224. 246. 253-255. 259.261. 265. 296. 300. 303. 305. 312-313.364. 408. 416. 423-424. 426-427. 571.573-5741657-415. 275

---. 1658-298. 183. 2651659-487 (GX 339-4). 265. 324-326.330. 332. 3391700-377. 2751702-363 (GX 349+2). 265. 324-326.330. 332. 3391702-429. 256. 265. 3421705-250. 2651705-440. 183. 265. 326-327. 333.338. 3391715-321. 2651722-363. 2751724-307.266.534, 5481728-169 (GX 9+9). 183. 266. 308.326. 339. 340-3411728-247 (GX 1+4),259.261. 266. 5741728-337 (GX 354-0). 266. 326. 339.533-5341730-335 (Rapid Burster) 255. 257. 266.478.5331731-260. 2661732-30. 2661735-444. 183. 248. 266. 308. 323.326-327. 333, 337-339. 533. 5431741-293 (MXB 1743-29).2671742-289 (MXB 1743-29). 267. 5341742-294 (MXB 1742-29).2671743-28. 2671744-265 (GX 3+1). 267, 326, 333-335,339-341. 5331744-300, 2671745-203. 2671745-247, 267. 5331746-331. 2671746-370. 2681747-214, 2681755-338. 183. 268. 302. 3041758-205 (GX 9+1). 268. 326. 339-3411758-250 (GX 5-1). 268. 322-326. 330.334-335. 337-338. 450-452. 467-469.475

591

1811-171 (GX 13+1). 2681812-12. 2681813-140 (GX 17+2). 183,268.325-326. 330-332. 339. 341. 453.1820-303. 183. 198. 201-202. 269.326-327. 333. 335. 338-339. 341. 5331822-371. 175. 183. 198. 202. 269.299-302. 304-3051833-076 (Set X-I). 2751836-04, 2751837-t{)49 (Ser X-I). 269. 339. 341. 5431843+00. 2761843-024. 2761850-087. 269. 5341905+000. 269, 5331907+097. 2761908+005 (Aql X-I). 269. 503. 533.5431909-t{)48. 2761916-053. 183. 269. 304. 5331936+541. 2761956+350 (Cyg X-I). 245. 276, 340.502.5481957+115, 183. 269. 3081EI048.1. 574lE1145.1. 5741E2259+59. 5742000+25. 269. 3122023+338. 2702030+375, 254, 276. 366. 424. 4682030+407 (Cyg X-3). 33. 183. 198-199.202. 204, 207. 246. 270, 308-309. 339.3412127+119. 183. 2702129+470, 175. 183, 270. 300-301.304-306, 3122137+57 (Cep X-4). 2762142+380 (Cyg X-2),175, 183. 185.209, 211-212. 245, 260, 270. 310.323-326. 330-332. 335-339, 447-452.462-465, 469. 475-4762202+501, 2772206+543. 2772214+589. 277AC 211. 201-202. 309accretion driven. 245eclipsing. 246flaring branch. 259, 261galactic. 245-246galactic bulge, 247. 486GCX-1. 339. 341

592

---, horizontal branch, 259. 260---, In accreting neutron stars, 366. 374, 385.

407---. In globular clusters, 247. 252

LS lt61° 303, 297M5 1603+26, 183normal branch, 259photospheric radius expansion, 25855 433N1343 Aqr. 296X Per, 374XOO21.8-7221. 574

X-ray transients. 543hard. 501

---. soft, 247, 251, 298-299, 310-313,501-513ultrasoft, 501-503

Z sources, 260, 319-320, 322-328, 334classification of, 325, 336-341low frequency noise, 334optical emission, 337power spectra of, 329-332radio emission, 337UV emission, 337