Spectrophotometry of eight bright Be stars

Details Spectrophotometry of eight bright Be stars Spectrophotometry of eight bright Be stars

Jun 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...180..167g&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 180, no. 1-2, June 1987, p. 167-171.

Astronomy and Astrophysics

Astrophysics

3

B Stars, Spectral Energy Distribution, Stellar Spectrophotometry, Stellar Temperature, Astronomical Models, Monochromatic Radiation, Near Infrared Radiation, Near Ultraviolet Radiation

Scientific paper

New continuum energy distribution data of eight Be stars are presented in the region λλ3200 - 8000 Å. Spectrophotometric measurements for five of the eight Be stars, are presented for the first time. The effective temperatures of these stars have been estimated by comparing the observed continuum energy distribution curves with theoretical model atmospheres. Near-ultraviolet and near-infrared excess is found to be present in five Be stars.

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