aas, lb 01/06 press conf -1 a plethora of pulsars roger w. romani stanford university alice k....

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LB 01/06 Press Conf -1 A A Plethora Plethora of of Pulsars Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

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Page 1: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -1

A A PlethoraPlethora of Pulsars of Pulsars

Roger W. Romani

Stanford University

Alice K. Harding

GSFC

for the

Fermi LAT collaboration

Page 2: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -2

Fermi LAT Pulsar Discoveries

• We announce today the discovery of 12 new pulsars found directly in the gamma-rays and 17 additional pulsars seen for the first time as gamma-ray emitters.

• In the first 4 months of the mission, over 3 dozen pulsars detected!– confirmed 6 known EGRET pulsars (and several EGRET candidates)

– Found 12 new young radio pulsars

– Found 13 young pulsars pulsing in Gamma-rays alone

– Found 7 ‘Millisecond’ Gamma-ray pulsars

• This harvest tells us many things:– A unique probe into the heart of the pulsar machine

– A new, less biased look at the fate of massive stars

Page 3: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -3

w/ New Fermi LAT Pulsar DiscoveriesGamma Only

MSP

Radio+Gamma

-Ray Pulsars Known Before Today

Page 4: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -4

The Pulsing -ray Sky

Pulses at1/10th true rate

Page 5: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -5

-only Pulsars:High Altitude Emission

Traditional Polar CapEmission

High Altitude GapEmission

Conclusion: LAT -ray PSRdiscoveries kill the classical Polar Cap picture

Page 6: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -6

What Pulses? Depends on where you look:

• Basic outer gap predictions

– Radio along B axis– -ray along equator

• 4 Possible cases– Both: Radio + -ray PSR

• Most famous objects

– Radio-only PSR• fainter slot gap ?

– Neither: no Radio, no -ray • Thermal X-ray only

• Hard to find!

– Gamma: -ray only• Geminga, CTA-1

Page 7: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -7

Fermi Probes the PowerAnd now I see, with eye serenethe very pulse of the machine;

--Wm Wordsworth “She was a Phantom of Delight”

Log

(P

ower

Rad

iate

d)

Log (Photon Energy)

Radio

Fermi -ray >10,000x

Radio X-ray -ray

Page 8: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -8

Gamma-Ray Millisecond Pulsars with Gamma-Ray Millisecond Pulsars with the Fermi Large Area Telescopethe Fermi Large Area Telescope

• First clear detection of -ray pulsations from a millisecond pulsar – 7 found

• New population of -ray pulsars has been

established

Alice K. HardingNASA Goddard Space Flight

for the

Fermi LAT Collaboration

Page 9: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -9

ms ms -ray pulsars-ray pulsars

• Very different characteristics from the normal -ray pulsars:– Spinning 100 times

faster– Magnetic fields

~10,000 times lower– ~10,000 times older

• “Recycled” pulsars spun-up by binary companion stars

Page 10: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -10

Spin-up of a millisecond pulsar

Page 11: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -11

Millisecond Millisecond -ray pulses-ray pulses

Fermi -ray

Radio

PRELIMINARY

Page 12: AAS, LB 01/06 Press Conf -1 A Plethora of Pulsars Roger W. Romani Stanford University Alice K. Harding GSFC for the Fermi LAT collaboration

AAS, LB 01/06 Press Conf -12

Summary pointsSummary points

• Millisecond pulsars pulse in -rays!• Six new-ray ms pulsars discovered with Fermi• EGRET low-significance candidate (PSR J0218+4232)

confirmed

• Old recycled pulsars can accelerate particles to very high (TeV) energies

• Fermi is seeing so far the nearby ms pulsar population

• This may be the tip-of-the-iceberg with many more to be discovered