The maximum possible velocity of dynamically ejected runaway stars
A total of 9550 point particle binary-binary scattering experiments have been performed in order to estimate the maximum possible velocity (MPV) of dynamically ejected runaway stars. It is found that the MPV for a low-mass companion ejected from a binary-binary interaction is roughly the escape velo...
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Veröffentlicht in: | The Astronomical journal 1991-02, Vol.101 (2), p.562-571 |
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description | A total of 9550 point particle binary-binary scattering experiments have been performed in order to estimate the maximum possible velocity (MPV) of dynamically ejected runaway stars. It is found that the MPV for a low-mass companion ejected from a binary-binary interaction is roughly the escape velocity from the surface of the most massive star involved in the interaction. The MPV at infinity that the most massive star involved in an interaction can attain is roughly half the escape velocity from the star's surface. (C.D.) |
doi_str_mv | 10.1086/115704 |
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T</creatorcontrib><title>The maximum possible velocity of dynamically ejected runaway stars</title><title>The Astronomical journal</title><description>A total of 9550 point particle binary-binary scattering experiments have been performed in order to estimate the maximum possible velocity (MPV) of dynamically ejected runaway stars. It is found that the MPV for a low-mass companion ejected from a binary-binary interaction is roughly the escape velocity from the surface of the most massive star involved in the interaction. The MPV at infinity that the most massive star involved in an interaction can attain is roughly half the escape velocity from the star's surface. (C.D.)</description><subject>Astronomy</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Stellar dynamics and kinematics</subject><subject>Stellar systems. Galactic and extragalactic objects and systems. 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T</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>The maximum possible velocity of dynamically ejected runaway stars</atitle><jtitle>The Astronomical journal</jtitle><date>1991-02-01</date><risdate>1991</risdate><volume>101</volume><issue>2</issue><spage>562</spage><epage>571</epage><pages>562-571</pages><issn>0004-6256</issn><eissn>1538-3881</eissn><coden>ANJOAA</coden><abstract>A total of 9550 point particle binary-binary scattering experiments have been performed in order to estimate the maximum possible velocity (MPV) of dynamically ejected runaway stars. It is found that the MPV for a low-mass companion ejected from a binary-binary interaction is roughly the escape velocity from the surface of the most massive star involved in the interaction. The MPV at infinity that the most massive star involved in an interaction can attain is roughly half the escape velocity from the star's surface. 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source | Elektronische Zeitschriftenbibliothek - Frei zugängliche E-Journals; Alma/SFX Local Collection |
subjects | Astronomy Earth, ocean, space Exact sciences and technology Stellar dynamics and kinematics Stellar systems. Galactic and extragalactic objects and systems. The universe |
title | The maximum possible velocity of dynamically ejected runaway stars |
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