1999A&AS..138..505D

Query : 1999A&AS..138..505D

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

Full paper

View the references in ADS

Number of rows : 5

N	Identifier	Otype	ICRS (J2000) RA	ICRS (J2000) DEC	Mag B	Sp type	#ref 1850 - 2023	#notes
1	GRB 970228	gB	05 01 46.7	+11 46 53		~	634	1
2	GBS 1900+14	gB	19 07 13	+09 19.6		~	834	0
3	SNR G042.8+00.6	SNR	19 07 41.80	+09 07 17.0		~	126	1
4	Granat 1915+105	HXB	19 15 11.55576	+10 56 44.9052		~	2504	0
5	SN 1998bw	SN*	19 35 03.17	-52 50 46.1	14.09	SNIc	1767	2

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