Emission of Continuum Radiation from Bright Be Stars
Corresponding Author(s) : P. S. GORAYA
paramjitgoraya@yahoo.com
Asian Journal of Chemistry,
Vol. 18 No. 5 (2006): Vol 18 Issue 5
Abstract
Continuum radiation distribution observations of Be stars are presented in the wavelength region 3200-8000Å. The effective temperature of Be stars are derived by comparing the observed energy distribution curves with the theoretical models. Various peculiarities detected in Be stars are discussed. Three Be stars are found to possess near-UV and near-IR excess radiation emission.
Keywords
Be stars
Energy distribution
Excess emission
S. GORAYA, P. (2010). Emission of Continuum Radiation from Bright Be Stars. Asian Journal of Chemistry, 18(5), 3306–3309. Retrieved from https://asianpubs.org/index.php/ajchem/article/view/13847
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