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Detection of X-rays from Algol /beta Persei/X-rays in the 2-6 keV band were detected from the Algol system using the rotating modulation collimator system on SAS-3 during an observation in October 1975. The measured X-ray flux is 3.8 x 10 to the -11th ergs/sq cm/s/keV. No positive detection was made in the 6-11 keV band. The data are consistent with either a power-law spectrum with photon spectral index not less than 2.5 or a thermal bremsstrahlung spectrum with a temperature not greater than 3 x 10 to the 7th K.
Document ID
19770033184
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Schnopper, H. W.
(Harvard Coll. Observatory Cambridge, MA, United States)
Delvaille, J. P.
(Harvard Coll. Observatory Cambridge, MA, United States)
Epstein, A.
(Harvard Coll. Observatory Cambridge, MA, United States)
Helmken, H.
(Harvard Coll. Observatory Cambridge, MA, United States)
Murray, S. S.
(Harvard College Observatory and Smithsonian Astrophysical Observatory Cambridge, Mass., United States)
Clark, G.
(Harvard Coll. Observatory Cambridge, MA, United States)
Jernigan, G.
(Harvard Coll. Observatory Cambridge, MA, United States)
Doxsey, R.
(MIT Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
December 1, 1976
Publication Information
Publication: Astrophysical Journal
Volume: 210
Subject Category
Astrophysics
Accession Number
77A16036
Funding Number(s)
CONTRACT_GRANT: NAS5-11450
Distribution Limits
Public
Copyright
Other

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