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CPD -48 deg 1577 - The brightest known cataclysmic variableThe discovery is reported of a V = 9.4 mag star which has the properties of a cataclysmic variable. Its UBV colors are similar to those of UX UMa, and its brightness fickers with an amplitude of the order of 0.1 mag. Larger brightness variations (0.5 mag) are found on a time scale of years. Its spectrum is characterized by extremely weak absorption lines of He I and He II, as well as extremely broad, shallow lines of H. A broad K line is very weakly present in absorption. Emission cores with a very slow decrement are seen in the H lines. From a comparison with the known properties of other cataclysmic variables, the distance, reddening, and mass exchange rate are estimated. The space density of cataclysmic variables is also estimated, since the original spectroscopic survey is complete to magnitude B = 10.0.
Document ID
19840037730
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Krzeminski, W.
(Las Campanas Observatory La Serena, Chile)
Garrison, R. F.
(Las Campanas Observatory Chile)
Schild, R. E.
(Las Campanas Observatory Chile)
Hiltner, W. A.
(Las Campanas Observatory Chile)
Date Acquired
August 12, 2013
Publication Date
January 1, 1984
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 276
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
84A20517
Funding Number(s)
CONTRACT_GRANT: NGR-23-005-464
Distribution Limits
Public
Copyright
Other

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