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Spectrophotometric study of X Persei
Authors:B B Sanwal  B S Rautela  S C Joshi
Institution:(1) Uttar Pradesh State Observatory, Naini Tal, India
Abstract:The continuum energy distribution of the emission line star X Per (O9.5III-V) has been obtained in the wavelength range 340–710 nm and has been compared with the energy distribution of agr Cam in the same wavelength range. The continuum of the star is found to be modified by the circumstellar envelope. A number density of the order of 1011 in the envelope has been obtained from the observations of Hagr in emission.
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