Spectrophotometric observations of HR 8107

Details Spectrophotometric observations of HR 8107 Spectrophotometric observations of HR 8107

Mar 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989japa...10..113j&link_type=abstract

Journal of Astrophysics and Astronomy (ISSN 0250-6335), vol. 10, March 1989, p. 113-118.

Astronomy and Astrophysics

Astrophysics

B Stars, Spectral Energy Distribution, Stellar Spectrophotometry, Stellar Temperature, Stellar Atmospheres, Stellar Luminosity, Stellar Spectra

Scientific paper

HR 8107, a reported new Be star, has been observed spectrophotometrically. The energy distribution curve of the star has been compared with those of other stars of similar spectral and luminosity types and model atmospheres. On the basis of comparison with model atmospheres an effective temperature has been assigned to the star.

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