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Bright-rimmed clouds with IRAS point sources: candidates for star formation by radiation-driven implosion

Published online by Cambridge University Press:  03 August 2017

Koji Sugitani ,
Yasuo Fukui  and
Katsuo Ogura
Koji Sugitani
Affiliation:
I. Physikalisches Institut, Universität zu Köln College of General Education, Nagoya City University
Yasuo Fukui
Affiliation:
Department of Astrophysics, Nagoya University
Katsuo Ogura
Affiliation:
Kokugakuin University

Extract

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We present preliminary results of a survey of bright-rimmed clouds associated with IRAS point sources.

Bright-rimmed globules associated with old HII regions have long been suspected as a potential site for star formation. Physical conditions of such clouds seem to well match to models of radiation-driven implosion, which have been studied as an effective process for induced star formation (e.g. Klein et al. 1985, Bertoldi 1989). Bright-rimmed globules associated with IRAS point sources are good candidates for the sites of induced star formation. Three well-established cases of radiation-driven implosions in bright-rimmed globules (Ori I-2, IC1396-n, and L1206) were reported (Sugitani et al. 1989). Similar examples were also reported in HH46/47 (Olberg et al. 1989) and in GN21.38.9 (Duvert et al. 1990). However, the samples are still not numerous enough to establish comprehensive understanding of star formation by such implosion process.

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 498 - 499
Copyright
Copyright © Kluwer 1991 

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