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Connection between the Star Formation Rate and the Gamma-Ray Bursts

Published online by Cambridge University Press:  21 March 2013

Attila Mészáros ,
Zsolt Bagoly ,
Lajos G. Balázs  and
István Horváth
Attila Mészáros
Affiliation:
Faculty of Mathematics and Physics, Astronomical Institute, Charles University, V Holešovičkách 2, CZ 180 00 Prague 8, Czech Republic, email: meszaros@cesnet.cz
Zsolt Bagoly
Affiliation:
Department of Physics of Complex Systems, Eötvös University, H-1117 Budapest, Pázmány P. s. 1/A, Hungary
Lajos G. Balázs
Affiliation:
Konkoly Observatory, H-1505 Budapest, POB 67, Hungary
István Horváth
Affiliation:
Department of Physics, Bolyai Military University, H-1581 Budapest, POB 15, Hungary
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Abstract

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It is remarkable that the long gamma-ray bursts, as objects connected with the supernovae - i.e. with the end of the massive stars, trace the star formation rate. This connection is discussed in this contribution. The presentation is in essence a recapitulation of the article Mészáros A. et al. A&A, 2006, 455, 785.

Keywords

gamma rays: bursts — supernovae: general — stars: formation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S292: Molecular Gas, Dust, and Star Formation in Galaxies , August 2012 , pp. 334
Copyright
Copyright © International Astronomical Union 2013

References

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Madau, P. 1995, ApJ, 441, 18CrossRefGoogle Scholar
Mészáros, A., Bagoly, Z., Balázs, L. G., & Horváth, I. 2006, A&A, 455, 785Google Scholar
Řípa, J., Mészáros, A., Veres, P., & Park, I. H. 2012, ApJ, 756, 44Google Scholar