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Extracting Velocities for Faint Secondaries

Published online by Cambridge University Press:  12 April 2016

D. Cohen
Affiliation:
Department of Astronomy, University of Wisconsin, 475 Charter Street, Madison, Wisconsin 53706, USA and Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA
D.W. Latham
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA

Abstract

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When velocities can be determined for both members of a double-lined spectroscopic binary, then the mass ratio can be calculated immediately. With the goal of measuring velocities for faint secondaries in single-lined spectroscopic binaries, we have experimented with a technique of first subtracting the spectrum of the primary using synthetic spectra calculated from Kurucz model stellar atmospheres and then correlating to get the velocity of the secondary. For half a dozen of the single-lined spectroscopic binaries in the Carney-Latham survey of proper-motion stars we have been able to extract velocities for the secondaries and to solve for double-lined orbits.

Type
Spectroscopic Studies
Copyright
Copyright © Astronomical Society of the Pacific 1992

References

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