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Radio Continuum around NGC 7538–IRS 1

Published online by Cambridge University Press:  25 April 2016

K. Akabane ,
M. Inoue ,
R. Kawabe ,
N. Ohashi ,
O. Kamaya ,
M. Ishiguro  and
Y. Sofue
K. Akabane
Affiliation:
Department of Physics, Toyama University, Gofuku, Toyama, Japan
M. Inoue
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano, Japan
R. Kawabe
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano, Japan
N. Ohashi
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano, Japan
O. Kamaya
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano, Japan
M. Ishiguro
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano, Japan
Y. Sofue
Affiliation:
Institute of Astronomy, University of Tokyo, Mitaka, Tokyo, Japan
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Abstract

We report continuum observations of the NGC 7538–IRS 1, 2 and 3 regions made with the NRO 45-metre dish between 43 and 90 GHz, and present a brief interpretation.

Type
Galactic and Stellar
Information
Publications of the Astronomical Society of Australia , Volume 9 , Issue 1 , 1991 , pp. 118 - 119
Copyright
Copyright © Astronomical Society of Australia 1991

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References

Campbell, B., 1984, Astrophys. J. Lett., 282, L27.Google Scholar
Martin, A. H. M., 1973, Mon. Not. R. Astr. Soc., 163, 141.Google Scholar
Scoville, N. Z. et al., 1986, Astrophys. J., 303, 416.CrossRefGoogle Scholar