Relations between U, B, V intrinsic colours and Geneva photometry for B-type stars - The effective temperature scales

Details Relations between U, B, V intrinsic colours and Geneva photometry for B-type stars - The effective temperature scales Relations between U, B, V intrinsic colours and Geneva photometry for B-type stars - The effective temperature scales

Mar 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...132..283c&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 132, no. 2, March 1984, p. 283-290.

Astronomy and Astrophysics

Astrophysics

53

B Stars, Stellar Color, Stellar Spectrophotometry, Stellar Temperature, Calibrating, Ubv Spectra

Scientific paper

The relations linking the Geneva and Johnson U, B, V intrinsic colours of B-type stars of classes V to III are defined via estimators based on the Geneva reddening-free X and Y parameters. These estimators allow the direct intercomparison of the properties of these three photometric frameworks of analysis. A new Teff vs. X relation is defined and, in a first application of the relations above, is compared with existing Teff vs. Johnson (U, B, V)0 relations.

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