The Eclipsing Double-Lined Spectroscopic Binary System V505 Persei

Authors

Laurence A. Marschall, Gettysburg CollegeFollow
Robert P. Stefanik, Harvard-Smithsonian Center for AstrophysicsFollow
Claud H. Lacy, University of ArkansasFollow
Guillermo Torres, Harvard-Smithsonian Center for AstrophysicsFollow
David B. Williams
Franz Agerer

Document Type

Article

Publication Date

8-1997

Department 1

Physics

Abstract

The recently-discovered eclipsing double-lined spectroscopic binary V505 Persei (SAO 23229) consists of two nearly identical F5 main sequence stars in a 4.2 day orbit. We have obtained both spectroscopic and photometric observations of the binary that densely sample the complete cycle of radial velocity and light variations. These observations have been used to determine the elements of the orbit, to determine individual masses of the stars in the system to a precision of better than 1%, and to estimate an age for the system. The derived properties agree well with current stellar structure models and provide fundamental data for tests of stellar evolution theory.

Copyright Note

This is the publisher's version of the work. This publication appears in Gettysburg College's institutional repository by permission of the copyright owner for personal use, not for redistribution.

DOI

10.1086/118511

Recommended Citation

Marschall, Laurence A. et al. The Eclipsing Double-Lined Spectroscopic Binary System V505 Persei. The Astronomical Journal (August 1997) 114(2): 793-799.

Required Publisher's Statement

Original version available from the publisher at: http://iopscience.iop.org/1538-3881