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Dynamical activity in V1016 CygniNew high-dispersion IUE observations show the C IV emission lines in V1016 Cygni to be split, suggesting evidence for dynamical activity. The Mg V line shows structure nearly identical to the C IV lines when plotted in velocity space.
Document ID
19850053289
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1086/184464
Authors
Feibelman, W. A. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Fahey, R. P. (NASA Goddard Space Flight Center Laboratory for Astronomy and Solar Physics, Greenbelt, MD, United States)
Date Acquired
August 12, 2013
Publication Date
May 1, 1985
Publication Information
Publication: Astrophysical Journal, Part 2 - Letters to the Editor
Volume: 292
ISSN: 0004-637X
Subject Category
Astrophysics
Report/Patent Number
ISSN: 0004-637X
Accession Number
85A35440
Distribution Limits
Public
Copyright
Other

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