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arXiv.org e-Print Archive
Preprint . 1997
Data sources: arXiv.org e-Print Archive
https://doi.org/10.1063/1.5538...
Article . 1998 . Peer-reviewed
Data sources: Crossref
https://dx.doi.org/10.48550/ar...
Article . 1997
License: arXiv Non-Exclusive Distribution
Data sources: Datacite
https://dx.doi.org/10.1063/1.5...
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Properties of GRB host galaxies

descriptionPublicationkeyboard_double_arrow_right Article , Preprint , Other literature type 01 Jan 1998Embargo end date: 01 Jan 1997 United States Publisher:ASCEJournal:Fourth Huntsville gamma-ray burst symposium
Authors: Hartmann, Dieter H.; Band, David L.;

doi: 10.1063/1.55388 , 10.48550/arxiv.astro-ph/9712125

arXiv: astro-ph/9712125

Properties of GRB host galaxies

Abstract

The transients following GRB970228 and GRB970508 showed that these (and probably all) GRBs are cosmological. However, the host galaxies expected to be associated with these and other bursts are largely absent, indicating that either bursts are further than expected or the host galaxies are underluminous. This apparent discrepancy does not invalidate the cosmological hypothesis, but instead host galaxy observations can test more sophisticated models.

5 pages, AIPPROC LaTeX, to appear in "Gamma-Ray Bursts, 4th Huntsville Symposium," eds. C. Meegan, R. Preece and T. Koshut

Country
United States
Related Organizations
Keywords

Astrophysics (astro-ph), FOS: Physical sciences, Astrophysics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
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