Continuum energy dissipation of 48 Persei

Details Continuum energy dissipation of 48 Persei Continuum energy dissipation of 48 Persei

Dec 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987ap%26ss.139..257t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 139, no. 2, Dec. 1987, p. 257-262.

Astronomy and Astrophysics

Astrophysics

Continuous Spectra, Emission Spectra, Energy Dissipation, Spectral Energy Distribution, Stellar Spectra, Variable Stars, Infrared Radiation, Interstellar Extinction, Stellar Spectrophotometry, Ultraviolet Radiation

Scientific paper

Continuum energy distribution data for 48 Per are given in the 3200-8000 A optical region and are supplemented by data in the ultraviolet and infrared wavelength range. 48 Per is shown to exhibit an ultraviolet deficiency as compared to a normal B-star. The results also indicate an infrared excess emission in 48 Per. A T(eff) value is obtained which is much higher than the value expected from a star of this spectral type, possibly due to the increased opacity of the envelope and the resulting near-ultraviolet and near-infrared deficiency.

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