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SiO in Star Forming Regions: Barnard 1 and Orion KL

Published online by Cambridge University Press:  12 April 2016

Satoshi Yamamoto ,
Hitomi Mikami  and
Shuji Saito
Satoshi Yamamoto
Affiliation:
Department of Astrophysics, Nagoya University, Chikusa, Nagoya 464-01, Japan
Hitomi Mikami
Affiliation:
Department of Astrophysics, Nagoya University, Chikusa, Nagoya 464-01, Japan
Shuji Saito
Affiliation:
Institute for Molecular Science, Okazaki 444, Japan

Abstract

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Interferometric observations of the SiO (J = 2 − 1) line are carried out toward a low-mass-star forming region, Bl, and a massive star forming region, Ori KL. Production mechanisms of SiO in these regions are discussed.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 243 - 244
Copyright
Copyright © Astronomical Society of the Pacific 1994

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