Teff for B, A and F main sequence stars (Sokolov, 1995)

Details Teff for B, A and F main sequence stars (Sokolov, 1995) Teff for B, A and F main sequence stars (Sokolov, 1995)

Jan 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ycat..41100553s&link_type=abstract

VizieR On-line Data Catalog: J/A+AS/110/553. Originally published in: 1995A&AS..110..553S

Physics

Spectrophotometry, Ultraviolet, Stars: B-Type, Stars: A-Type, Stars: F-Type, Effective Temperatures

Scientific paper

A method of determination of the effective temperature of B, A and F
main sequence stars is proposed, using the slope of the continuum
between 3200A and 3600A. We have determined the Balmer jump and the
effective temperatures for 235 main sequence stars. (1 data file).

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