Spectrophotometric study of X Persei

Details Spectrophotometric study of X Persei Spectrophotometric study of X Persei

Mar 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.110..301s&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 110, no. 2, March 1985, p. 301-309.

Astronomy and Astrophysics

Astrophysics

1

B Stars, M Stars, O Stars, Star Clusters, Stellar Envelopes, Stellar Spectrophotometry, Astronomical Catalogs, Density Distribution, Emission Spectra, H Alpha Line, Interstellar Extinction, Spectral Energy Distribution, Supergiant Stars, Wavelengths

Scientific paper

The continuum energy distribution of the emission line star X Per (O9.5 III-V) has been obtained in the wavelength range 340 - 710 nm and has been compared with the energy distribution of α 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 Hα in emission.

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