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Line profile variation in delta-Orionis A, l-Orionis A, and 15 MonocerotisThe results of a monitoring program with IUE and Einstein are presented for three stars, delta-Ori A, l-Ori A, and 15 Mon. Line profile variability is observed in the UV profiles accessible to IUE and the relation between the variation in the different ions suggests that the ionization level is varying in the winds of these stars. This is consistent with Einstein observations of soft X-ray variability for two of the stars.
Document ID
19840064415
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Grady, C. A.
(Colorado, University Boulder, CO; Sonnenobservatorium Einsteinturm, Potsdam, East Germany; Computer Sciences Corp., Falls, United States)
Snow, T. P.
(Colorado Univ. Boulder, CO, United States)
Cash, W. C.
(Colorado, University Boulder, CO; Sonnenobservatorium Einsteinturm, Potsdam, Germany)
Date Acquired
August 12, 2013
Publication Date
August 1, 1984
Publication Information
Publication: Astrophysical Journal, Part 1
Volume: 283
ISSN: 0004-637X
Subject Category
Astrophysics
Accession Number
84A47202
Funding Number(s)
CONTRACT_GRANT: NAG8-327
CONTRACT_GRANT: NSG-5300
CONTRACT_GRANT: NAS5-26409
Distribution Limits
Public
Copyright
Other

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