Publikationsdatum:
2011-08-19
Beschreibung:
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.
Schlagwort(e):
ASTROPHYSICS
Materialart:
Astrophysical Journal, Part 2 - Letters to the Editor (ISSN 0004-637X); 292; L15-L18
Format:
text