Fundamental parameters of fast-rotating B stars (Fremat+, 2005)

Details Fundamental parameters of fast-rotating B stars (Fremat+, 2005) Fundamental parameters of fast-rotating B stars (Fremat+, 2005)

Jul 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006ycat..34400305f&link_type=abstract

VizieR On-line Data Catalog: J/A+A/440/305. Originally published in: 2005A&A...440..305F

Astronomy and Astrophysics

Astronomy

Models: Atmosphere, Stars: Early-Type

Scientific paper

The reference model parameters proper to calculating FASTROT rotationally modified synthetic spectra, as well as those obtained by fitting the rotationally distorted spectra with them, are hereafter called parent non-rotating counterpart (pnrc) fundamental parameters, while vsini will represent the true projected rotation velocity of the star. Conversely, we call apparent fundamental parameters (e.g. TeffA, loggA and vsiniA), those derived by fitting the GRIDB spectral lines with synthetic spectra issued from classical plane-parallel model atmospheres.
(1 data file).

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