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A. Young
© 1975. The Astronomical Society of the Pacific. All rights reserved. Printed in U.S.A.
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Citation A. Young 1975 PASP 87 717
DOI 10.1086/129833
72 Total downloads
Spectroscopic orbital elements are derived for the eclipsing binary IQ Per. Faint secondary lines are detected, and a mass ratio and individual masses are inferred. The components are found to be on the main sequence, and the system is detached. Key words: eclipsing binary - radial velocities - orbit
