Hostname: page-component-78c5997874-g7gxr Total loading time: 0 Render date: 2024-11-02T19:07:22.396Z Has data issue: false hasContentIssue false
  • English
  • Français

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

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.

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

Campbell, B. 1984, Astrophys.J.Letters, 282, L27.Google Scholar
Davidson, K., and Harwit, M. 1967, Astrophys.J., 95, 1185.Google Scholar
Turner, B.E., and Matthews, H.E. 1984, Astrophys.J., 277, 164.Google Scholar