The problem of normal energy distribution in stellar spectra - A0-A2 main-sequence stars

Details The problem of normal energy distribution in stellar spectra - A0-A2 main-sequence stars The problem of normal energy distribution in stellar spectra - A0-A2 main-sequence stars

Aug 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..760k&link_type=abstract

Astronomicheskij Zhurnal, vol. 70, p. 760

Astronomy and Astrophysics

Astronomy

8

A Stars, Stellar Spectra, Spectral Energy Distribution, Interstellar Extinction, Astronomical Interferometry

Scientific paper

The normal energy distribution in the range 3200-7600 A is presented for two sources of spectral classification data. The spectrophotometric data are taken from three catalogs (B-V) and (U-B) indices for all A0-A2V normal stars from the Bright Star Catalog are analyzed to estimate the sufficiency of the present sample of stars for characterizing each subclass. The average (B-V) and (U-B) indices are calculated for these subclasses.

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