Pulsar's kicks and Gamma-ray bursts - INSPIRE

DataBETA

Pulsar's kicks and Gamma-ray bursts

Jan, 2007

3 pages

Published in:

Astron.Astrophys. 472 (2007) 1

e-Print:

astro-ph/0701888 [astro-ph]

DOI:

10.1051/0004-6361:20077200

View in:

ADS Abstract Service

reference search8 citations

Citations per year

Abstract: (arXiv)

The supernova-GRB (Gamma-ray burst) association is tested by showing the consistence of the distributions of pulsar's kick velocities and GRB energies, under the assumption that cosmic GRBs are related to supernova explosions that form pulsars. These two distributions are derived from observations, and are checked by K-S test. The deduced distribution of kick velocity from the total energy of GRBs and the observed distribution of radio pulsars are found to come from a same parent population. This result may indicate that GRBs could be really related to supernovae, and that the asymmetry of GRB fireballs would cause the kick of pulsars.

Note:

Submitted to Astron.Astrophys.

STARS NEUTRON
DENSE MATTER

References(36)

Figures(0)

BATSE observations of gamma-ray burst spectra. 1. Spectral diversity.

D. Band
(
- UC, San Diego and
- NASA, Goddard and
- Alabama U., Huntsville
)
,
J. Matteson
(
- UC, San Diego and
- NASA, Goddard and
- Alabama U., Huntsville
)
,
L. Ford
(
- UC, San Diego and
- NASA, Goddard and
- Alabama U., Huntsville
)
,
B. Schaefer
(
- UC, San Diego and
- NASA, Goddard and
- Alabama U., Huntsville
)
,
D. Palmer
(
- UC, San Diego and
- NASA, Goddard and
- Alabama U., Huntsville
)

et al.

- Astrophys.J. 413 (1993) 281-292
•
DOI:
- 10.1086/172995

The prompt energy release of gamma-ray bursts using a cosmological k-correction

- Astron.J. 121 (2001) 2879-2888
•
e-Print:
- astro-ph/0102371
•
DOI:
- 10.1086/321093

Improved models of stellar core collapse and still no explosions: What is missing?

- Phys.Rev.Lett. 90 (2003) 241101
•
e-Print:
- astro-ph/0303171
•
DOI:
- 10.1103/PhysRevLett.90.241101

- Phys.Rev.Lett. 76 353

The Birth of Quark Stars: Photon-driven Supernovae?

Anbo Chen
(
- Peking U.
)
,
Renxin Xu
(
- Peking U.
)

- Astrophys.J.Lett. 668 (2007) L55
•
e-Print:
- astro-ph/0605285
•
DOI:
- 10.1086/522777

Neutron star population dynamics. 2. 3-D space velocities of young pulsars

- Astrophys.J. 505 (1998) 315-338
•
e-Print:
- astro-ph/9707308
•
DOI:
- 10.1086/306138

Gamma-ray bursts and afterglows from rotating strange stars and neutron stars

Z.G. Dai
(
- Nanjing U.
)
,
T. Lu
(
- Nanjing U.
)

- Phys.Rev.Lett. 81 (1998) 4301-4304
•
e-Print:
- astro-ph/9810332
•
DOI:
- 10.1103/PhysRevLett.81.4301

Galactic gamma-ray bursters: The Cosmic ray sources at all energies

Arnon Dar
(
- Technion and
- Munich, Max Planck Inst.
)
,
Rainer Plaga
(
- Munich, Max Planck Inst.
)

- Astron.Astrophys. 349 (1999) 259-266
•
e-Print:
- astro-ph/9902138

Transition to Quark Matter and long Gamma Ray Bursts

- Nuovo Cim.B 121 (2006) 1355-1361
•
e-Print:
- astro-ph/0701240
•
DOI:
- 10.1393/ncb/i2007-10265-2

The Collimation-corrected GRB energies correlate with the peak energy of their nu f_ nu spectrum

G. Ghirlanda
(
- Brera Observ.
)
,
G. Ghisellini
(
- Brera Observ.
)
,
D. Lazzati
(
- Cambridge U., Inst. of Astron.
)

- Astrophys.J. 616 (2004) 331-338
•
e-Print:
- astro-ph/0405602
•
DOI:
- 10.1086/424913

- Astron.J. 160 979

The Pulsar kick velocity distribution

Brad M.S. Hansen
(
- Canadian Inst. Theor. Astrophys. and
- Caltech
)
,
E.Sterl Phinney
(
- Caltech
)

- Mon.Not.Roy.Astron.Soc. 291 (1997) 569
•
e-Print:
- astro-ph/9708071
•
DOI:
- 10.1093/mnras/291.3.569

Long Gamma Ray Bursts from Quark Stars

- Nuovo Cim.B 121 (2006) 1349-1354
•
e-Print:
- astro-ph/0701258
•
DOI:
- 10.1393/ncb/i2007-10257-2

VLA observations of broad 6-cm excited state OH lines in W49a

- Mon.Not.Roy.Astron.Soc. 360 (2005) 993-1006
•
e-Print:
- astro-ph/0504117
•
DOI:
- 10.1111/j.1365-2966.2005.09085.x

Gamma-ray bursts from neutron star kicks

Y.F. Huang
(
- Nanjing U., Dept. Astron. and
- Beijing, Inst. High Energy Phys.
)
,
Z.G. Dai
(
- Nanjing U., Dept. Astron.
)
,
T. Lu
(
- Nanjing U., Dept. Astron.
)
,
K.S. Cheng
(
- Hong Kong U.
)
,
X.F. Wu
(
- Nanjing U., Dept. Astron.
)

- Astrophys.J. 594 (2003) 919-923
•
e-Print:
- astro-ph/0303365
•
DOI:
- 10.1086/377129

The Central engine of gamma-ray bursters

W. Kluzniak
(
- Wisconsin U., Madison and
- Warsaw, Copernicus Astron. Ctr.
)
,
M. Ruderman
(
- Columbia U. and
- IAS, Rome
)

- Astrophys.J.Lett. 505 (1998) L113-L117
•
e-Print:
- astro-ph/9712320
•
DOI:
- 10.1086/311622

Spin orbit interaction in neutron star / main sequence binaries and implications for pulsar timing

Dong Lai
(
- Caltech
)
,
Lars Bildsten
(
- UC, Berkeley and
- UC, Berkeley, Astron. Dept.
)
,
Victoria M. Kaspi
(
- Caltech, JPL
)

- Astrophys.J. 452 (1995) 819
•
e-Print:
- astro-ph/9505042
•
DOI:
- 10.1086/176350

Orbital decay of the psr j0045-7319/b star binary system: age of radio pulsar and initial spin of neutron star

Dong Lai

- Astrophys.J.Lett. 466 (1996) L35
•
e-Print:
- astro-ph/9605096
•
DOI:
- 10.1086/310166

Pulsar jets: implications for neutron star kicks and initial spins

- Astrophys.J. 549 (2001) 1111
•
e-Print:
- astro-ph/0007272
•
DOI:
- 10.1086/319455

- Mon.Not.Roy.Astron.Soc. 289 592

- Mon.Not.Roy.Astron.Soc. 201 503

High birth velocities of radio pulsars

- Nature 369 (1994) 127
•
DOI:
- 10.1038/369127a0

A Neutron Star-driven XRF associated with SN 2006aj

et al.

- Nature 442 (2006) 1018-1020
•
e-Print:
- astro-ph/0603567
•
DOI:
- 10.1038/nature05081

The Core collapse supernova mechanism: Current models, gaps, and the road ahead

Anthony Mezzacappa
(
- Oak Ridge
)

- ASP Conf.Ser. 342 (2005) 175
•
e-Print:
- astro-ph/0410085

The Core collapse supernova mechanism: Current models, gaps, and the road ahead

Anthony Mezzacappa
(
- Oak Ridge
)

- ASP Conf.Ser. 342 (2005) 175
•
e-Print:
- astro-ph/0410085

1-25 of 36
1
2
25 / page