Scanner observations of shell stars Phi Persei and Psi Persei

Details Scanner observations of shell stars Phi Persei and Psi Persei Scanner observations of shell stars Phi Persei and Psi Persei

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.143...99t&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 143, no. 1, April 1988, p. 99-105.

Astronomy and Astrophysics

Astrophysics

Hot Stars, Main Sequence Stars, Shell Stars, Spectral Energy Distribution, Spectrophotometry, Stellar Mass Ejection, Stellar Rotation, Emission Spectra, H Alpha Line, Line Spectra, Stellar Temperature

Scientific paper

Spectrophotometric energy distribution data of the shell stars φ Per and ψ Per are reported in the wavelength range λλ3200 - 8000 Å. The effective temperature of these stars is derived by comparison of observed energy distribution with theoretical models. Both the stars show higher values of derived effective temperature. The continuum energy distribution in the ultraviolet region has also been discussed.

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