Continuum energy distributions of some bright Be stars

Details Continuum energy distributions of some bright Be stars Continuum energy distributions of some bright Be stars

Sep 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984a%26a...138...19g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 138, no. 1, Sept. 1984, p. 19-24.

Astronomy and Astrophysics

Astrophysics

24

B Stars, Early Stars, Spectral Energy Distribution, Stellar Evolution, Stellar Temperature, Atmospheric Models, Stellar Atmospheres, Stellar Models, Stellar Rotation, Ubv Spectra

Scientific paper

The absolute flux distributions of seven bright Be stars, in the wavelength range λλ350 - 750 nm is presented. The observed energy distribution curves are compared with Kurucz (1979) model atmospheres to estimate their effective temperatures. Some peculiarities in the energy distributions and the evolutionary stages of the Be stars are discussed.

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