1999A&AS..138..505D


C.D.S. - SIMBAD4 rel 1.7 - 2021.05.07CEST15:00:27

1999A&AS..138..505D - Astron. Astrophys., Suppl. Ser., 138, 505-506 (1999/September-0)

Jetted GRBs, afterglows and SGRs from quark stars birth.

DAR A.

Abstract (from CDS):

A phenomenological model is presented to explain the light curves of gamma-ray bursts. Gamma-rays are produced in a narrow beam which sweeps through space due to the precession of a slaved accretion disc. The light curve expected from such a precessing luminosity cone can explain the complex temporal behavior of bright gamma-ray bursts.

Abstract Copyright:

Journal keyword(s): accretion discs - black hole physics - binaries: close - stars: neutron - gamma-rays: bursts - gamma-rays: theory

Simbad objects: 5

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Number of rows : 5

N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
#notes
1 GRB 970228 gB 05 01 46.7 +11 46 53           ~ 627 1
2 GBS 1900+14 gB 19 07 13 +09 19.6           ~ 801 0
3 SNR G042.8+00.6 SNR 19 07 41.80 +09 07 17.0           ~ 122 1
4 Granat 1915+105 HXB 19 15 11.55576 +10 56 44.9052           ~ 2364 0
5 SN 1998bw SN* 19 35 03.17 -52 50 46.1   14.09       SNIc 1685 2

    Equat.    Gal    SGal    Ecl

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2021.05.07-15:00:27

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