The Origin of OB Runaway Stars-Reference-Cited by-同舟云学术

The Origin of OB Runaway Stars

Published:2011-12-09 Issue:6061 Volume:334 Page:1380-1383
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Fujii Michiko S.¹²,Zwart Simon Portegies¹

Affiliation:

1. Leiden Observatory, Leiden University, Post Office. Box 9513, 2300 RA Leiden, Netherlands.

2. Graduate School of Science and Engineering, Kagoshima University, 1-21-35 Korimoto, Kagoshima 890-0065, Japan.

Abstract

Most of the unusually fast, young stars in our Galaxy are produced in three-body encounters within dense clusters of stars.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference54 articles.

1. The Space Motions of AE Aurigae and μ Columbae with Respect to the Orion Nebula.

2. The binary frequency and origin of the OB runaway stars

3. On the origin of the O- and B-type stars with high velocities (the ”runaway” stars), and some related problems;Blaauw A.;Bull. Astron. Inst. Neth.,1961

4. Runaway stars from young star clusters containing initial binaries. I - Equal-mass, equal-energy binaries

5. Binary Evolution in Stellar Dynamics

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