Spectrophotometry of some Be stars

Details Spectrophotometry of some Be stars Spectrophotometry of some Be stars

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986ap%26ss.120..133s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 120, no. 1, March 1986, p. 133-138.

Astronomy and Astrophysics

Astrophysics

2

B Stars, Infrared Stars, Stellar Spectrophotometry, Balmer Series, Continuous Spectra, Emission Spectra, Spectral Energy Distribution, Stellar Magnitude, Stellar Temperature, Variable Stars

Scientific paper

The continuum energy distributions of six Be stars, namely 25 Cyg, 31 Peg, HR 8758, 14 Lac, 12 Vul, and β Psc, in the wavelength region λλ3200 - 7800 Å, are presented. Comparing the observed energy distributions with those of theoretical models given by Kurucz (1979), their effective temperatures are determined. A near-infrared excess emission at wavelengths above λ6000 Å is seen in most of the stars.

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