Hostname: page-component-78c5997874-dh8gc Total loading time: 0 Render date: 2024-11-04T21:00:56.481Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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

References

Bachiller, R., Martín-Pintado, J., and Fuente, A., 1991, A&A, 243, L21.Google Scholar
Bachillet, R., Menten, K.M., and del Rio-Alvarez, S., 1990, A&A, 236, 461.Google Scholar
Mangum, J.G. et al., 1990, ApJ, 348, 542.Google Scholar
Mikami, H. et al., 1992, ApJ, 392, L87.Google Scholar
Nakayama, M., 1988, M.S. Thesis, Tohoku Univ.Google Scholar
Wright, M.C.H., et al., ApJ, 267, L41.Google Scholar
Yamamoto, S. et al., 1992, PASJ, 44, 459.Google Scholar
Yamamoto, S., Mikami, H., and Saito, S., 1993, in this proceeding.Google Scholar
Ziurys, L.M., Friberg, P., Irvine, W.M., 1989, ApJ, 343, 201.Google Scholar