Intrinsic Energy Distributions in Spectra of Early Type Stars

Details Intrinsic Energy Distributions in Spectra of Early Type Stars Intrinsic Energy Distributions in Spectra of Early Type Stars

Oct 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990mnras.246..408p&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Vol. 246, NO. 3/OCT1, P. 408, 1990

Astronomy and Astrophysics

Astronomy

17

Scientific paper

The intrinsic energy distributions in the spectra of stars hotter than B5 are derived from the TD-1 data samples as mean distributions, averaged for some spectral types over more than 100 stars. The `peculiarities' resulting from incorrect classifications or errors in recording the data have been detected and excluded from the samples. The new set of intrinsic (B-V)0 colours, differing slightly from the existing ones is proposed. The derived spectrophotometric standards are apparently free of reddening effects in visual and far-UV segments of their spectra. The set of stars proposed as natural standards is also included.

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