IUE and La-Silla Observations of Mass Loss in the Magellanic Clouds

Details IUE and La-Silla Observations of Mass Loss in the Magellanic Clouds IUE and La-Silla Observations of Mass Loss in the Magellanic Clouds

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980msngr..21....4m&link_type=abstract

The Messenger, No.21, P. 4, 1980

Computer Science

Scientific paper

The phenomenon of mass-Ioss in hot stars has been known for a good many years. The strong stellar winds which are the manifestation of this phenomenon are observed as broad emission lines in the spectra of hot stars. In a number of cases the emission is red-shifted from the laboratory wavelength and a blue shifted absorption component appears; this is the so-calied "P-Cygni" line profile as it was first seen in the spectrum of the star P Cygni.

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