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Optical Spectroscopy of V635 Cassiopeiae/4U 0115+63In this paper we present two data sets that can be used to constrain the physical and geometric models for the circumstellar disk. The companion's spectral type is a critical parameter for modelling the disk.
Document ID
20060041143
Acquisition Source
Jet Propulsion Laboratory
Document Type
Reprint (Version printed in journal)
External Source(s)
hdl:2014/19056
Authors
Unger, S. J.
Roche, P.
Negueruela, I.
Ringwald, F. A.
Lloyd, C.
Coe, M. J.
Date Acquired
August 23, 2013
Publication Date
March 1, 1998
Publication Information
Publication: Astronomy and Astrophysics
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Other
Keywords
stars circumstellar matter emission line binary neutron stars

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