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PX269 Galaxies Part 2: Our Galaxy, the Milky Way 2.1 Components and Structure PX269 Galaxies
PX269 Galaxies Part 2: Our Galaxy, the Milky Way 2.1 Components and Structure PX269 Galaxies
224 views
Development of a depository in an analytical facility –– a sample-preservation mission Tak Kunihiro, Y. Yachi, H. Kitagawa, and E. Nakamura Pheasant Memorial
Development of a depository in an analytical facility –– a sample-preservation mission Tak Kunihiro, Y. Yachi, H. Kitagawa, and E. Nakamura Pheasant Memorial
213 views
Ch.4. Broad Line Region broad lines are important to understand AGN structure for at least two reasons: 1) BLR motions are almost certainly determined
Ch.4. Broad Line Region broad lines are important to understand AGN structure for at least two reasons: 1) BLR motions are almost certainly determined
221 views
AFM-Raman and Tip Enhanced Raman studies of modern nanostructures Pavel Dorozhkin, Alexey Shchekin, Victor Bykov NT-MDT Co., Build. 167, Zelenograd Moscow,
AFM-Raman and Tip Enhanced Raman studies of modern nanostructures Pavel Dorozhkin, Alexey Shchekin, Victor Bykov NT-MDT Co., Build. 167, Zelenograd Moscow,
221 views
Chandra Calibration Status ACIS 1.Gain correction files for epochs 30, 31 and 32 were released in CALDB 3.4.1 (Sept 2007), 3.4.2 (Dec. 2007) and 3.4.3
Chandra Calibration Status ACIS 1.Gain correction files for epochs 30, 31 and 32 were released in CALDB 3.4.1 (Sept 2007), 3.4.2 (Dec. 2007) and 3.4.3
216 views
Microphysics of the radiative transfer. Numerical integration of RT in a simplest case Local Thermodynamical Equilibrium (LTE, all microprocesses are
Microphysics of the radiative transfer. Numerical integration of RT in a simplest case Local Thermodynamical Equilibrium (LTE, all microprocesses are
216 views
Magnetic Fields at Mt. Wilson and MDI. The 150-foot Tower Spectrograph Measures 12 line pairs simultaneously The long-term program uses 5250. The full
Magnetic Fields at Mt. Wilson and MDI. The 150-foot Tower Spectrograph Measures 12 line pairs simultaneously The long-term program uses 5250. The full
221 views
Finding Photospheric Flows with I+LCT or,“Everything you always wanted to know about velocity at the photosphere, but were afraid to ask.” B. T. Welsch,
Finding Photospheric Flows with I+LCT or,“Everything you always wanted to know about velocity at the photosphere, but were afraid to ask.” B. T. Welsch,
214 views
SHINE 2008
SHINE 2008
45 views
AFM-Raman and Tip Enhanced Raman studies of modern nanostructures
AFM-Raman and Tip Enhanced Raman studies of modern nanostructures
33 views
Measuring the black hole spin of GX 339-4: A systematic look at its very high and low/hard state. Rubens Reis Institute of Astronomy - Cambridge In collaboration
Measuring the black hole spin of GX 339-4: A systematic look at its very high and low/hard state. Rubens Reis Institute of Astronomy - Cambridge In collaboration
213 views
Complex Epitaxial Oxides: Synthesis and Scanning Probe Microscopy Goutam Sheet, 1 Udai Raj Singh, 2 Anjan K. Gupta, 2 Ho Won Jang, 3 Chang-Beom Eom 3 and
Complex Epitaxial Oxides: Synthesis and Scanning Probe Microscopy Goutam Sheet, 1 Udai Raj Singh, 2 Anjan K. Gupta, 2 Ho Won Jang, 3 Chang-Beom Eom 3 and
220 views