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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

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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

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