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Interstellar C2 molecules toward Zeta OphiuchiTen weak interstellar absorption lines of the (2-0) Phillips band of C2 near 8760 A are detected in the spectrum of Zeta Ophiuchi. All of the lines have equivalent widths smaller than 2 mA, and originate from the six lowest rotational levels of C2. The resulting total column density is equal to about 1.7 x 10 to the 13th/sq cm, and the excitation temperature is 130 + or - 10 K.
Document ID
19820043812
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Hobbs, L. M.
(Yerkes Observatory Williams Bay, WI, United States)
Campbell, B.
(Canada-France-Hawaii Telescope Corp. Kamuela, HI, United States)
Date Acquired
August 10, 2013
Publication Date
March 1, 1982
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
82A27347
Funding Number(s)
CONTRACT_GRANT: NGR-14-001-147
Distribution Limits
Public
Copyright
Other

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