The lambda Boo stars - A reappraisal

Details The lambda Boo stars - A reappraisal The lambda Boo stars - A reappraisal

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...127..231h&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 127, no. 1, Oct. 1983, p. 231-234. Research supported by the Swiss National Sc

Astronomy and Astrophysics

Astrophysics

35

A Stars, Peculiar Stars, Stellar Spectrophotometry, Early Stars, F Stars, Hertzsprung-Russell Diagram, Stellar Color, Stellar Spectra

Scientific paper

The class of peculiar stars called λ Boo stars consists of a
small number of metal weak-lined A-F stars. The authors suggest a
spectroscopic definition of this group and study the properties of the
nine stars so defined in the Geneva and uvby β photometric systems.
Their metal deficiency appears clearly in both systems.

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