Hostname: page-component-cd9895bd7-dk4vv Total loading time: 0 Render date: 2024-12-26T03:25:11.359Z Has data issue: false hasContentIssue false

A Study of the Spectrum of the OH Megamaser in III Zw 351

Published online by Cambridge University Press:  12 April 2016

Zhi-yao Yu*
Affiliation:
Shanghai Astronomical Observatory and Union Laboratory of Radio Astronomy, The Chinese Academy of Science, 80 Nandan Road, Shanghai 200030, China

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.

III Zw 35 is an OH megamaser galaxy which is of great interest. In this paper, the spectrum has been fitted and the position map has been studied. A new model of multiple and distinct rotating and expanding rings in a thin disk is proposed in this paper.

Type
VIII. Megamasers in Active Galaxies
Copyright
Copyright © Astronomical Society of the Pacific 1997

Footnotes

1

This work is supported by the National Natural Science Foundation of China.

References

Baan, W.A., 1990, ApJ, 364, 65.Google Scholar
Baan, W.A., Haschick, A.D., & Henkel, C. 1989, ApJ, 346, 680.Google Scholar
Carroll, T.J., & Kwan, J. 1985, ApJ, 288, 73.Google Scholar
Chapman, J.M., et al. 1990, MNRAS, 244, 281.Google Scholar
Chevalier, R., & Clegg, A. 1985, Nature, 317, 44.CrossRefGoogle Scholar
Harwit, M., et al. 1987, ApJ, 315, 28.CrossRefGoogle Scholar
Montgomery, A.S., & Cohen, R.J. 1992, MNRAS, 254, 23p.Google Scholar
Staveley-Smith, L., et al. 1987, MNRAS, 226, 689.Google Scholar
Yu, Z.-Y. 1994, Acta Ap. Sinica, 14, 66.Google Scholar