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Spectroscopic survey of the far-ultraviolet /1160-1700 A/ emissions of CapellaA far-ultraviolet spectral survey of Capella (Alpha Aur, G5 III + G0 III) has been obtained using a highly sensitive rocketborne spectrograph with a microchannel plate detector. The spectral distribution is very similar to that of the sun; however, if the line surface fluxes are due to the primary (G5 III), then, except for Ly-alpha, they are about an order of magnitude greater than those of the quiet sun
Document ID
19760049062
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/182084
Authors
Vitz, R. C. (Johns Hopkins Univ. Baltimore, MD, United States)
Weiser, H. (Johns Hopkins Univ. Baltimore, MD, United States)
Moos, H. W. (Johns Hopkins Univ. Baltimore, MD, United States)
Weinstein, A. (Johns Hopkins Univ. Baltimore, MD, United States)
Warden, E. S. (Johns Hopkins University Baltimore, Md., United States)
Date Acquired
August 8, 2013
Publication Date
April 1, 1976
Publication Information
Publication: Astrophysical Journal
Volume: 205
Subject Category
Astronomy
Accession Number
76A32028
Funding Number(s)
CONTRACT_GRANT: NGR-21-001-001
Distribution Limits
Public
Copyright
Other

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