Hostname: page-component-586b7cd67f-t7fkt Total loading time: 0 Render date: 2024-11-29T13:32:28.941Z Has data issue: false hasContentIssue false
  • English
  • Français

Distribution of HC5N in IRC+10216

Published online by Cambridge University Press:  12 April 2016

Shuro Takano  and
Shuji Saito
Shuro Takano
Affiliation:
Institute for Molecular Science, Myodaiji, Okazaki, Japan 444
Shuji Saito
Affiliation:
Institute for Molecular Science, Myodaiji, Okazaki, Japan 444

Abstract

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.

The distribution of HC5N was observed in the envelope of the carbon star IRC+10216 with the Nobeyama Millimeter Array. A shell like distribution with its diameter of about 29″ was found. The diameter is larger than that of HC3N.

Type
3. Astronomical Results and Prospects
Information
International Astronomical Union Colloquium , Volume 140: Astronomy with Millimeter and Submillimeter Wave Interferometry , 1994 , pp. 150 - 151
Copyright
Copyright © Astronomical Society of the Pacific 1994

References

Bieging, J.H. and Nguyen-Q-Rieu, 1988, ApJ, 329, L107.Google Scholar
Bieging, J.H. and Tafalla, M. 1992, to appear in AJ.Google Scholar
Takano, S., Saito, S., and Tsuji, T. 1992, PASJ, 44, 469.Google Scholar
Zuckerman, B. and Aller, L.H. 1986, ApJ, 301, 772.Google Scholar