The UV spectrum of WZ SGE at nova maxium

Details The UV spectrum of WZ SGE at nova maxium The UV spectrum of WZ SGE at nova maxium

Apr 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980esasp.157...85f&link_type=abstract

The second European International Ultraviolet Explorer (IUE) Conference, held 26-28 March 1980 in Tübingen, West Germany. Edited

Astronomy and Astrophysics

Astronomy

1

Binary Stars, Iue, Novae, Stellar Mass Accretion, Ultraviolet Astronomy, Absorption Spectra, Carbon, Disks (Shapes), Emission Spectra, Helium, Photosphere, Silicon

Scientific paper

Profiles of relatively unblended lines on a short wavelength region high dispersion spectrum, were measured. Both line absorption and line emission are seen. The former is stellar and not interstellar. The profiles were classified, and their regions of formation are considered. The C 4 resonance blend can be understood as consisting of emission components having a similar profile to that of the He 2 1640 A, and black absorption lines. The form of the He 2 1640 A profile suggests moreover the existence of an outer excretion disk, in addition to the well-known accretion disk.

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