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- W3100234721 endingPage "142" @default.
- W3100234721 startingPage "111" @default.
- W3100234721 abstract "The galaxy population hosting long-duration GRBs provides a means to constrain the progenitor and an opportunity to use these violent explosions to characterize the nature of the high-redshift universe. Studies of GRB host galaxies in emission reveal a population of star-forming galaxies with great diversity, spanning a wide range of masses, metallicities, and redshifts. However, as a population GRB hosts are significantly less massive and poorer in metals than the hosts of other core-collapse transients, suggesting that GRB production is only efficient at metallicities significantly below Solar. GRBs may also prefer compact galaxies, and dense and/or central regions of galaxies, more than other types of core-collapse explosion. Meanwhile, studies of hosts in absorption against the luminous GRB optical afterglow provide a unique means of unveiling properties of the ISM in even the faintest and most distant galaxies; these observations are helping to constrain the chemical evolution of galaxies and the properties of interstellar dust out to very high redshifts. New ground- and space-based instrumentation, and the accumulation of larger and more carefully-selected samples, are continually enhancing our view of the GRB host population." @default.
- W3100234721 created "2020-11-23" @default.
- W3100234721 creator A5006309508 @default.
- W3100234721 creator A5028778207 @default.
- W3100234721 creator A5048353300 @default.
- W3100234721 creator A5066351733 @default.
- W3100234721 creator A5071700393 @default.
- W3100234721 date "2016-03-10" @default.
- W3100234721 modified "2023-10-17" @default.
- W3100234721 title "Long-Duration Gamma-Ray Burst Host Galaxies in Emission and Absorption" @default.
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