The Eclipsing Spectroscopic Binary System V505 Persei

Details The Eclipsing Spectroscopic Binary System V505 Persei The Eclipsing Spectroscopic Binary System V505 Persei

May 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aas...188.6007m&link_type=abstract

American Astronomical Society, 188th AAS Meeting, #60.07; Bulletin of the American Astronomical Society, Vol. 28, p.920

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Scientific paper

We have obtained extensive spectroscopic and photometric observations of the bright double-lined eclipsing binary V505 Persei (SAO 23229) discovered in 1989 by Kaiser. The system consists of two nearly identical F5 main sequence stars in a 4.2 day orbit. The observations enable us to derive high precision (<1%) values for the individual stellar masses, along with other properties of the binary system. These values agree well with current stellar structure models, and add to the growing base of fundamental stellar data applicable to tests of stellar evolution theory.

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