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The optical identification of 2A 0311-227 with a new AM Herculis-type objectThe X-ray source 2A 0311-227 has been precisely positioned by using the HEAO 1 scanning modulation collimator, resulting in an optical candidate with a B magnitude of about 15. Medium-resolution optical spectra of this star show remarkable similarity to the spectrum of AM Her, a short-period binary containing a magnetic white dwarf. The Balmer decrement in 2A 0311-227 is also similar to that in AM Her and may likewise be attributed to collisional excitation in a plasma with an electron density of the order of 10 to the 13th per cu cm.
Document ID
19790065676
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Griffiths, R. E.
(Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Chaisson, L.
(Harvard-Smithsonian Center for Astrophysics Cambridge, Mass., United States)
Ward, M. J.
(Cambridge University Cambridge, United Kingdom)
Blades, J. C.
(Anglo-Australian Observatory Epping, New South Wales, Australia)
Wilson, A. S.
(Maryland, University College Park, Md., United States)
Johnston, M. D.
(MIT Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
August 15, 1979
Publication Information
Publication: Astrophysical Journal
Subject Category
Astrophysics
Accession Number
79A49689
Funding Number(s)
CONTRACT_GRANT: NAS8-27972
CONTRACT_GRANT: NAS8-30543
Distribution Limits
Public
Copyright
Other

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