Radial velocities and orbital solution of the active binary star FG Ursae Majoris

Details Radial velocities and orbital solution of the active binary star FG Ursae Majoris Radial velocities and orbital solution of the active binary star FG Ursae Majoris

Jan 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002ibvs.5227....1m&link_type=abstract

Information Bulletin on Variable Stars, 5227, 1.

Astronomy and Astrophysics

Astrophysics

1

Active Binaries, Orbital Solutions

Scientific paper

The orbital parameters of the single-lined active binary FG UMa are
derived, for the first time, by analyzing medium-resolution spectra
collected at Catania Astrophysical Observatory from 1997 till 2000.
Radial velocities were measured by using the cross correlation
technique.

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