NASA NTRS · 19850053289
Dynamical activity in V1016 Cygni
Abstract
New 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.
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Feibelman, W. A., Fahey, R. P.. 1985-05-01. Dynamical activity in V1016 Cygni. https://ntrs.nasa.gov/citations/19850053289
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