Free Access
Issue
Astron. Astrophys. Suppl. Ser.
Volume 138, Number 3, September 1999
Gamma-Ray Bursts in the Afterglow Era Contents Rome, November 3-6, 1998
Page(s) 483 - 484
DOI https://doi.org/10.1051/aas:1999320
Published online 15 September 1999
DOI: 10.1051/aas:1999320



Astron. Astrophys. Suppl. Ser. 138, 483-484

Distribution of compact object mergers around galaxies

T. Bulik1 - K. Belczynski1 - W. Zbijewski2


1 - Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warszawa, Poland
2 - Department of Physics, University of Warsaw, Hoza 69, Warszawa, Poland

Received December 29, 1998; accepted April 21, 1999

Abstract:

Compact object mergers are one of the favoured models of gamma ray bursts (GRB). Using a binary population synthesis code we calculate properties of the population of compact object binaries; e.g. lifetimes and velocities. We then propagate them in galactic potentials and find their distribution in relation to the host.

Key words: gamma-rays: bursts -- stars: binaries; evolution

Copyright The European Southern Observatory (ESO)

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