2009ApJ...705L..15Y


Query : 2009ApJ...705L..15Y

2009ApJ...705L..15Y - Astrophys. J., 705, L15-L19 (2009/November-1)

Gamma-ray burst luminosity relations: two-dimensional versus three-dimensional correlations.

YU B., QI S. and LU T.

Abstract (from CDS):

The large scatters of luminosity relations of gamma-ray bursts (GRBs) have been one of the most important reasons that prevent the extensive applications of GRBs in cosmology. In this paper, we extend the two-dimensional (2D) luminosity relations with τlag, V, Epeak, and τRT as the luminosity indicators to three dimensions (3D) using the same set of luminosity indicators to explore the possibility of decreasing the intrinsic scatters. We find that, for the 3D luminosity relations between the luminosity and an energy scale (Epeak) and a timescale (τlag or τRT), their intrinsic scatters are considerably smaller than those of corresponding 2D luminosity relations. Enlightened by the result and the definition of the luminosity (energy released in units of time), we discussed possible reasons behind this result, which may give us helpful suggestions on seeking more precise luminosity relations for GRBs in the future.

Abstract Copyright: ∼

Journal keyword(s): gamma rays: bursts

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 Fermi bn090423330 gB 09 55 33.19 +18 08 57.7           ~ 392 0

Query : 2009ApJ...705L..15Y

Basic data :
Fermi bn090423330 -- Gamma-ray Burst
Other object types:
otypes_help
gB (2016ApJS,GRB,...)
ICRS coord. (ep=J2000) :
09 55 33.19 +18 08 57.7 [ ] D 2009GCN..9322....1R
FK4 coord. (ep=B1950 eq=1950) :
09 52 47.94 +18 23 12.5 [ ]
Gal coord. (ep=J2000) :
215.93507 +48.64970 [ ]
Radial velocity / Redshift / cz :
V(km/s) 292791 [~] / z(~) 8.2 [~] / cz 2458298 [~]
   D 2009GCN..9219....1T
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Identifiers (3) :
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GRB 090423 Fermi bn090423330 GRB 090423A

References (392 between 1850 and 2026) (Total 392)
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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