2006ApJ...646.1098Z


Query : 2006ApJ...646.1098Z

2006ApJ...646.1098Z - Astrophys. J., 646, 1098-1103 (2006/August-1)

Is GRB 050904 a superlong burst?

ZOU Y.C., DAI Z.G. and XU D.

Abstract (from CDS):

By considering synchrotron radiative process in the internal shock model and assuming that all internal shocks are nearly equally energetic, we analyze the gamma-ray burst (GRB) emission at different radii corresponding to different observed times. We apply this model to GRB 050904 and find that our analytical results can provide a natural explanation for the multiband observations of GRB 050904. This suggests that the X-ray flare emission and the optical emission of this burst could have originated from internal shocks due to collisions among nearly equally energetic shells ejected from the central engine. Thus, GRB 050904 appears to be a burst with superlong central engine activity.

Abstract Copyright: ∼

Journal keyword(s): Gamma Rays: Bursts - Hydrodynamics - Relativity - Shock Waves

Simbad objects: 1

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Number of rows : 1
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026
#notes
1 GRB 050904 gB 00 54 50.794 +14 05 09.42           ~ 496 0

Query : 2006ApJ...646.1098Z

Basic data :
GRB 050904 -- Gamma-ray Burst
Other object types:
otypes_help
gB (GRB), UV (2009ApJ)
ICRS coord. (ep=J2000) :
00 54 50.794 +14 05 09.42 (Ultraviolet) [ 2300 2300 90 ] D 2009ApJ...690..163R
FK4 coord. (ep=B1950 eq=1950) :
00 52 13.194 +13 48 54.43 [ 2300 2300 90 ]
Gal coord. (ep=J2000) :
124.186243 -48.777496 [ 2300 2300 90 ]
Radial velocity / Redshift / cz :
V(km/s) 288733 [600] / z(~) 6.295 [0.002] / cz 1887194 [600]
   D 2006ApJ...637L..69W
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Identifiers (1) :
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GRB 050904

References (496 between 1850 and 2026) (Total 496)
Simbad bibliographic survey began in 1850 for stars (at least bright stars) and in 1983 for all other objects (outside the solar system).
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