Continuum energy distribution of Be stars

Details Continuum energy distribution of Be stars Continuum energy distribution of Be stars

Jul 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.113..325s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 113, no. 2, July 1985, p. 325-331.

Astronomy and Astrophysics

Astrophysics

5

B Stars, Continuous Spectra, Spectral Energy Distribution, Stellar Spectra, Variable Stars, Interstellar Extinction, Stellar Spectrophotometry, Stellar Temperature

Scientific paper

The continuum energy distributions of four Be stars - namely, HR 7708, HR 7807, HR 7927, and HR 8171 alongwith two normal B stars HR 7426 and HR 7613 are presented in the wavelength region λλ3200 - 7800 Å. By comparing the observed continuum energy distributions with that of theoretical models given by Kurucz (1979), their effective temperatures are determined and discussed. The observed energy distribution curves show near infrared excess emission longward of λ6000 Å for HR 7807 and HR 8171 and a double Balmer jump for HR 7708.

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