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Millimeter-Wave Continuum Around NGC 7538-IRS1, IRS2, and IRS3

Published online by Cambridge University Press:  12 April 2016

Kenji Akabane ,
Shozo Tsunekawa ,
Makoto Inoue ,
Ryohei Kawabe ,
Nagayoshi Ohashi ,
Osamu Kameya ,
Masato Ishiguro  and
Yoshiaki Sofue
Kenji Akabane
Affiliation:
Department of Physics, Faculty of Science, Toyama University, 3190, Gofuku, Toyama, 930 Japan
Shozo Tsunekawa
Affiliation:
Department of Physics, Faculty of Science, Toyama University, 3190, Gofuku, Toyama, 930 Japan
Makoto Inoue
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano 384-13 Japan
Ryohei Kawabe
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano 384-13 Japan
Nagayoshi Ohashi
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano 384-13 Japan
Osamu Kameya
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano 384-13 Japan
Masato Ishiguro
Affiliation:
Nobeyama Radio Observatory, Minamimakimura Minamisakugun, Nagano 384-13 Japan
Yoshiaki Sofue
Affiliation:
Institute of Astronomy, The University of Tokyo, Mitaka, Tokyo 181

Extract

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Millimeter-wave continuum sources in NGC 7538 region were observed with the NRO 45-m telescope and Nobeyama Millimeter Array. NRO 45-m telescope observations showed that the compact region which includes IRS1, IRS2, and IRS3 has a strong millimeter-wave intensity excess, cf. figures 1, and 2.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 258 - 259
Copyright
Copyright © Astronomical Society of the Pacific 1994

References

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