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LGRB hosts in emission and in absorption

Published online by Cambridge University Press:  27 October 2016

Paul M. Vreeswijk
Paul M. Vreeswijk*
Affiliation:
Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot 7610001, Israel email: [email protected]
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Abstract

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Long-duration gamma-ray bursts (LGRBs) provide a unique way of selecting a sample of actively star-forming galaxies independent of their brightness and at practically any redshift. I will review what we know about the hosts and more immediate environments of LGRBs from two different perspectives: ultraviolet absorption-line spectroscopy of the bright early afterglow, and observations of their hosts in emission once the afterglow has faded away.

Keywords

Gamma rays: burstsISM: abundancesGalaxies: high-redshift
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , General Assembly A29B: Astronomy in Focus , August 2015 , pp. 244 - 245
Copyright
Copyright © International Astronomical Union 2016 

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