A spectral study of BM Orionis

Details A spectral study of BM Orionis A spectral study of BM Orionis

Oct 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988azh....65..971i&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 65, Sept.-Oct. 1988, p. 971-978. In Russian.

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Early Stars, Stellar Mass, Stellar Spectra, Stellar Structure, Emission Spectra, H Lines, Line Spectra, Orbital Elements, Radial Velocity, Stellar Motions

Scientific paper

Radial velocity curves for separate components of the system have been
constructed, and new orbital elements were determined. Increase of
central intensities of lines of both components at the nodes of the
orbit has been discovered. Variations in the atmosphere of the cool star
has been discovered. The secondary components could be a T Tauri star

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