Connection between the Star Formation Rate and the Gamma-Ray Bursts
The result's identifiers
Result code in IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F00216208%3A11320%2F13%3A10193114" target="_blank" >RIV/00216208:11320/13:10193114 - isvavai.cz</a>
Result on the web
<a href="http://dx.doi.org/10.1017/S1743921313004419" target="_blank" >http://dx.doi.org/10.1017/S1743921313004419</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1017/S1743921313004419" target="_blank" >10.1017/S1743921313004419</a>
Alternative languages
Result language
angličtina
Original language name
Connection between the Star Formation Rate and the Gamma-Ray Bursts
Original language description
It is remarkable that the long gamma-ray bursts, as objects connected with the supernovae - i.e. with the end-stages of massive stars, trace the star formation rate. This connection is discussed in this contribution. The presentation is in essence a recapitulation of the article by Mészáros et al. (2006).
Czech name
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Czech description
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Classification
Type
D - Article in proceedings
CEP classification
BN - Astronomy and celestial mechanics, astrophysics
OECD FORD branch
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Result continuities
Project
<a href="/en/project/GAP209%2F10%2F0734" target="_blank" >GAP209/10/0734: Gamma-ray bursts</a><br>
Continuities
Z - Vyzkumny zamer (s odkazem do CEZ)
Others
Publication year
2013
Confidentiality
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů
Data specific for result type
Article name in the collection
The Intriguing Life of Massive Galaxies, Proceedings of the International Astronomical Union, IAU Symposium, Volume 295
ISBN
978-1-107-03384-9
ISSN
1743-9213
e-ISSN
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Number of pages
1
Pages from-to
93
Publisher name
Cambridge University Press
Place of publication
Cambridge, United Kingdom
Event location
Beijing, China
Event date
Aug 27, 2012
Type of event by nationality
WRD - Celosvětová akce
UT code for WoS article
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