Elements of the spectroscopic orbit of V 448 Cygni

Details Elements of the spectroscopic orbit of V 448 Cygni Elements of the spectroscopic orbit of V 448 Cygni

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...94g&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, May-June 1986, p. 94-96. In Russian.

Computer Science

Binary Stars, Orbital Elements, Stellar Motions, Stellar Orbits, Anomalies, Radial Velocity, Stellar Mass, Stellar Spectra

Scientific paper

Elements of the orbit of the close binary star V 448 Cygni have been
reconsidered. It is shown that the anomaly of the radial velocity curve
of a more massive star of the system is due to a complicated structure
of line profiles. New values of masses of components of the system
differ greatly from those determined earlier.

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