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Speckle–Spectroscopic Studies of Late–Type Stars

Published online by Cambridge University Press:  12 April 2016

A. Tokovinin*
Affiliation:
Sternberg Astronomical Institute, 119899 Universitetsky Prosp., 13 Moscow, Russia

Abstract

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The existing and new observing techniques for combined speckle–spectroscopic studies of binary stars are briefly reviewed. The late–type dwarf stars are particularly rewarding since simultaneous spatial and spectroscopic resolution is possible for a large number of systems. A list of new candidates for the interferometric resolution is given. These studies can make an important contribution to the data on stellar masses and also provide some insight into the binary formation mechanisms when applied to multiple systems.

Type
High Resolution At Visual Wavelengths
Copyright
Copyright © Astronomical Society of the Pacific 1992

References

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