The very broad lines in the UV spectra of hot emission stars - A possible explanation

Details The very broad lines in the UV spectra of hot emission stars - A possible explanation The very broad lines in the UV spectra of hot emission stars - A possible explanation

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008pobeo..84..463d&link_type=abstract

Publications of the Astronomical Observatory of Belgrade, vol. 84, pp. 463-466

Astronomy and Astrophysics

Astronomy

1

Scientific paper

In some cases, the UV spectral lines of hot emission stars and quasars
have very large widths that can not be explained as the consequence of
rotational or random velocities. In this paper we present a new idea to
explain this phenomenon.

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