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VLA Imaging of Class I Methanol Masers at 7 mm with Angular Resolution

Published online by Cambridge University Press:  12 April 2016

V. I. Slysh  and
L. Kogan
V. I. Slysh
Affiliation:
Astro Space Center, Lebedev Physical Institute, Moscow, Russia
L. Kogan
Affiliation:
National Radio Astronomy Observatory, Soccoro, NM 87801, U.S.A.

Abstract

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Eight Class I methanol masers were imaged at 44 GHz with A–configuration of the VLA providing angular resolution 0″.2. The images show a distribution of unresolved maser spots forming pairs in simple structure sources, and a distribution of pair clusters in complex sources. We found that the maser pairs are associated with hot, dense gas cores of sub–stellar masses. In complex sources the cores were found over the whole extent of the host molecular clouds.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 255 - 256
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Menten, K.M. 1991. In Skylines, Proceedings of the Third Haystack Observatory Meeting, eds. Haschick, A.D. & Ho, P.T.P. (San Francisco: ASP), 119–136.Google Scholar
Plambeck, R.L., & Menten, K.M. 1990. ApJ, 364, 555–560.Google Scholar