The environments and hosts of neutron star mergers and short GRBs
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F67985815%3A_____%2F23%3A00582409" target="_blank" >RIV/67985815:_____/23:00582409 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S1743921322000941" target="_blank" >http://dx.doi.org/10.1017/S1743921322000941</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921322000941" target="_blank" >10.1017/S1743921322000941</a>
Alternative languages
Result language
angličtina
Original language name
The environments and hosts of neutron star mergers and short GRBs
Original language description
The hosts of binary neutron star (BNS) mergers and hence short GRBs are not only galaxies with old stellar populations, infact most short GRB hosts are at least mildly star-forming galaxies. According to theoretical studies of merger populations, both short and long merging time-scales are expected. The immediate environments of BNS mergers are not as directly related to the property of the progenitor system as for long GRBs, since the system usually travelled a significant distance from their birth place. However, studying the stellar population properties across the host can still give us vital information on the contribution of formation channels and on merger timescales. Here we review the properties of NS merger hosts in emission using integrated-light and resolved observations. The afterglows of short GRBs furthermore serve to study the interstellar medium in their host galaxies in absorption. We present our best example to date, GRB 160410A at z = 1.7, one of the highest redshift short GRBs.
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
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OECD FORD branch
10308 - Astronomy (including astrophysics,space science)
Result continuities
Project
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Continuities
I - Institucionalni podpora na dlouhodoby koncepcni rozvoj vyzkumne organizace
Others
Publication year
2023
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
Neutron Star Astrophysics at the Crossroads: Magnetars and the Multimessenger Revolution
ISBN
9781108490757
ISSN
1743-9213
e-ISSN
1743-9221
Number of pages
8
Pages from-to
43-50
Publisher name
Cambridge University Press
Place of publication
Cambridge
Event location
virtual
Event date
Nov 29, 2021
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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