Physical Parameters of Stars in Close Binaries Derived from Gaia Photometry

Details Physical Parameters of Stars in Close Binaries Derived from Gaia Photometry Physical Parameters of Stars in Close Binaries Derived from Gaia Photometry

Jan 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005esasp.576..607n&link_type=abstract

"Proceedings of the Gaia Symposium "The Three-Dimensional Universe with Gaia" (ESA SP-576). Held at the Observatoire de Paris-Me

Physics

1

Stars Interacting Binaries, Eclipsing Variables

Scientific paper

The physical parameters of ten eclipsing binaries (eight contact and two semi-detached) are derived by using ground-based photometric observations and Hipparcos/Tycho photometric data, which mimic the photometric observations that are expected to be obtained by Gaia. The results are compared and the achievable precision of the basic stellar parameters derived by Gaia photometry is discussed.

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