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Ultraviolet photometry and spectrophotometry of AlgolOAO-2 blue and UV light curves and spectrophotometric observations are used to establish effective temperatures and luminosities for the three components of the eclipsing Algol (beta Persei) system. An essentially complete energy distribution is given for Algol, and the fundamental properties - geometrical quantities, wavelength-dependent quantities and derived astrophysical quantities - are presented for the star.
Document ID
19760031424
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Eaton, J. A.
(Washburn Observatory Madison, Wis., United States)
Date Acquired
August 8, 2013
Publication Date
October 1, 1975
Publication Information
Publication: Astronomical Society of the Pacific
Subject Category
Astronomy
Accession Number
76A14390
Funding Number(s)
CONTRACT_GRANT: NAS5-1348
Distribution Limits
Public
Copyright
Other

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