1999A&AS..138..477S


Query : 1999A&AS..138..477S

1999A&AS..138..477S - Astron. Astrophys., Suppl. Ser., 138, 477-478 (1999/September-0)

Severe new limits on the host galaxies of Gamma-Ray Bursts.

SCHAEFER B.E.

Abstract (from CDS):

Most burst models require bursters to reside in normal host galaxies with peak luminosities of L=1x1057photon/s or L=2x1058photon/s. These models can be directly tested by looking for host galaxies in small GRB error boxes in either of two data sets: (1) 8 optical transients detected for SAX bursts and (2) 23 of the all-time bright bursts. If the hosts are normal galaxies, then analysis of either data set shows L>6x1058photon/s. This result strongly rejects both luminosity cases provided bursters appear in normal host galaxies, with the bright burst sample being free of problems relating to galaxy evolution. In conclusion, bursters are either more distant than allowed for in the star-formation-rate scenario or they are not in normal galaxies.

Abstract Copyright: ∼

Journal keyword(s): gamma-rays: bursts

Simbad objects: 9

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Number of rows : 9
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 970228 gB 05 01 46.7 +11 46 53           ~ 650 1
2 GRB 970508 gB 06 53 49.2 +79 16 19           ~ 883 1
3 GRB 980329 gB 07 02 41 +38 50.7           ~ 276 1
4 GRB 980326 gB 08 36 34.3 -18 51 24           ~ 268 0
5 GRB 980613 gB 10 17 57.8 +71 27 26           ~ 204 1
6 GRB 971214 gB 11 56 26.4 +65 12 01           ~ 445 1
7 GRB 980519 gB 23 22 21.5 +77 15 43           ~ 203 0
8 GRB 980703 gB 23 59 06.7 +08 35 07           ~ 453 1
9 GRB 970425 gB ~ ~           ~ 3 0

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