Weak emission lines and peculiar stars

Details Weak emission lines and peculiar stars Weak emission lines and peculiar stars

Apr 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008coska..38..279w&link_type=abstract

Contributions of the Astronomical Observatory Skalnaté Pleso, vol. 38, no. 2, p. 279-284.

Astronomy and Astrophysics

Astronomy

1

Stars: B-Type, Stars: Chemically Peculiar, Spectral Lines: Emission

Scientific paper

Weak emission lines (WELs) of metals are observed in sharp-lined spectra of mid- to late-B type stars. The WELs are detected over a range of element abundance and are found among both chemically-normal and chemically-peculiar stars. The characteristics of this ubiquitous phenomenon are reviewed and their potential for the study of inhomogeneous stellar atmospheres is presented.

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