The constant orbital period of FF Ursae Majoris

Details The constant orbital period of FF Ursae Majoris The constant orbital period of FF Ursae Majoris

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012a%26a...537a..56g&link_type=abstract

Astronomy & Astrophysics, Volume 537, id.A56

Astronomy and Astrophysics

Astrophysics

Stars: Late-Type, Binaries: Spectroscopic, Stars: Individual: Ff Uma

Scientific paper

Gálvez et al. (2007, A&A, 472, 587) proposed that FF UMa, a
double-lined G-type spectroscopic binary, has a variable orbital period.
Here they are shown to be mistaken.

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