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Paschen beta emission in the spectrum of Omicron Ceti.Evaluation of three infrared spectra of Omicron Ceti obtained on Aug. 7 to 11, 1969. The equivalent width of the Paschen beta emission line in these spectra was found to vary by a factor of 2 during this time period. The variation was similar to that for H gamma and H delta as measured by Odell et al. (1970) for the same time span. The equivalent widths of Paschen beta and H gamma on August 7 were used to estimate an opacity ratio of kappa (1.28 micron)/kappa (0.43 micron) about equal to 1:30 and a molecular/atomic hydrogen ratio of about 10. The variation in the strength of Paschen beta and H delta lines is considered to be intrinsic and to have a time scale of less than or about equal to 100,000 sec.
Document ID
19720042013
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kovar, R. P.
Potter, A. E.
(NASA Manned Spacecraft Center Houston, Tex., United States)
Kovar, N. S.
(Houston, University Houston, Tex., United States)
Trafton, L.
(Texas, University Austin, Tex., United States)
Date Acquired
August 6, 2013
Publication Date
February 1, 1972
Publication Information
Publication: Astronomical Society of the Pacific
Subject Category
Space Sciences
Accession Number
72A25679
Distribution Limits
Public
Copyright
Other

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