UBVJHK synthetic photometry of Galactic O stars (Martins+, 2006)

Details UBVJHK synthetic photometry of Galactic O stars (Martins+, 2006) UBVJHK synthetic photometry of Galactic O stars (Martins+, 2006)

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34570637m&link_type=abstract

VizieR On-line Data Catalog: J/A+A/457/637. Originally published in: 2006A&A...457..637M

Physics

Stars: Early-Type, Stars: O, Models: Atmosphere, Photometry: Ubv, Photometry: Infrared

Scientific paper

Here, we derive UBVJHK magnitudes and bolometric corrections from a grid of atmosphere models for O stars. Bessel passbands are used. Bolometric corrections (BC) are derived as a function of Teff and are subsequently used to derive BC-spectral type (ST) and absolute magnitudes-ST relations.
(2 data files).

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