Identification of λ7887 Band of C2H2 in the Spectra of Two Carbon Stars 19 Psc and Y CVn
Author:
Affiliation:
1. Department of Geoscience, Fukuoka University of Education
Publisher
Japan Academy
Subject
General Medicine
Link
https://www.jstage.jst.go.jp/article/pjab1945/50/9/50_9_743/_pdf
Reference14 articles.
1. Davis, S. P., and Phillips, J. G. (1963): The Red System (A2Π-X2∑) of the CN Molecules. Univ. of California Press.
2. Fujita, Y., Yamashita, Y., and Tsuji, T. (1964): Proc. Japan Acad., 40, 664.
3. Fujita, Y., Tsuji, T., and Maehara, H. (1966): Proc. Japan Acad., 42, 765.
4. Fujita, Y. (1968): Bull. Astron. Inst. Czech., 19, 274.
5. Funke, G. W. (1937): Z. Phys., 104, 169.
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1. Identification of HCN in Carbon Stars;Proceedings of the Japan Academy, Series B;1983
2. Interpretation of the acetylene spectrum at 1.5 μm;Journal of Molecular Spectroscopy;1977-11
3. Calcium chloride in cool stars;Monthly Notices of the Royal Astronomical Society;1977-07-01
4. Carbon star photometry : CO and 3.2 micron bands.;The Astrophysical Journal;1976-02
5. Possible Presence of HCN in HD182040;Proceedings of the Japan Academy;1976
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