Spectral observations of Be stars in the visible range. I - Phi Per, Psi Per, 11 Cam, and Phi And

Details Spectral observations of Be stars in the visible range. I - Phi Per, Psi Per, 11 Cam, and Phi And Spectral observations of Be stars in the visible range. I - Phi Per, Psi Per, 11 Cam, and Phi And

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...43k&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Jan.-Feb. 1986, p. 43-47. In Russian.

Computer Science

6

B Stars, Stellar Spectra, Visible Spectrum, Balmer Series, Emission Spectra, H Alpha Line, H Beta Line

Scientific paper

Phi Per was found to display considerable variations of emission in H-alpha and H-beta. The H-alpha and H-beta emission profiles of Psi Per appeared to vary with a period of several years. A complete disappearance of H-alpha emission was observed for 11 Cam. Finally, the H-alpha emission for Phi And did not display intensity variations during the entire period of observations in 1983.

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