Distribution of compact object mergers around galaxies

T. Bulik; K. Belczyński; W. Zbijewski

doi:10.1051/aas:1999320

Distribution of compact object mergers around galaxies

T. Bulik, K. Belczyński, W. Zbijewski

Research output: Contribution to journal › Article › peer-review

6 Scopus citations

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.

Original language	English (US)
Pages (from-to)	483-484
Number of pages	2
Journal	Astronomy and Astrophysics Supplement Series
Volume	138
Issue number	3
DOIs	https://doi.org/10.1051/aas:1999320
State	Published - Sep 1999
Externally published	Yes

Keywords

Gamma-rays: bursts
Stars: binaries; evolution

ASJC Scopus subject areas

Physics and Astronomy(all)

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10.1051/aas:1999320

Cite this

@article{467a8f8e0a6c4e849739b9932c76f34f,

title = "Distribution of compact object mergers around galaxies",

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.",

keywords = "Gamma-rays: bursts, Stars: binaries; evolution",

author = "T. Bulik and K. Belczy{\'n}ski and W. Zbijewski",

year = "1999",

month = sep,

doi = "10.1051/aas:1999320",

language = "English (US)",

volume = "138",

pages = "483--484",

journal = "Astronomy and Astrophysics Supplement Series",

issn = "0365-0138",

publisher = "EDP Sciences",

number = "3",

}

TY - JOUR

T1 - Distribution of compact object mergers around galaxies

AU - Bulik, T.

AU - Belczyński, K.

AU - Zbijewski, W.

PY - 1999/9

Y1 - 1999/9

N2 - 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.

AB - 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.

KW - Gamma-rays: bursts

KW - Stars: binaries; evolution

UR - http://www.scopus.com/inward/record.url?scp=4244086763&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=4244086763&partnerID=8YFLogxK

U2 - 10.1051/aas:1999320

DO - 10.1051/aas:1999320

M3 - Article

AN - SCOPUS:4244086763

SN - 0365-0138

VL - 138

SP - 483

EP - 484

JO - Astronomy and Astrophysics Supplement Series

JF - Astronomy and Astrophysics Supplement Series

IS - 3

ER -

Distribution of compact object mergers around galaxies

Abstract

Keywords

ASJC Scopus subject areas

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