Resolution of the C IV+Fe III blend at 1550 A. II - The predominance of C IV in stars hotter than B1

Details Resolution of the C IV+Fe III blend at 1550 A. II - The predominance of C IV in stars hotter than B1 Resolution of the C IV+Fe III blend at 1550 A. II - The predominance of C IV in stars hotter than B1

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979a%26a....72..374b&link_type=abstract

Astronomy and Astrophysics, vol. 72, no. 3, Feb. 1979, p. 374, 375.

Astronomy and Astrophysics

Astrophysics

3

B Stars, Stellar Spectra, Supergiant Stars, Ultraviolet Spectra, Carbon, Early Stars, Hot Stars, Iron, Main Sequence Stars, Stellar Winds

Scientific paper

Copernicus scans in the region 1520-1560 A show that for six B0.5 and B0
stars the contribution of the C IV doublet increases with stellar
temperature and higher luminosity. P Cygni profiles are strong in the
spectra of supergiants and weakly visible in one main-sequence star.

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