Abstract
The evidence for mass loss in close binaries provided by spectroscopic observations is of two types; there is evidence for the existence of gaseous streams from one of the components and also for the existence of envelopes that surround a number of systems.
Member of the Carrera del Investigador Científico, Consejo Nacional de Investigationes Científicas y Técnicas, Argentina.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsAuthor information
Authors and Affiliations
Editor information
Rights and permissions
Copyright information
© 1969 D. Reidel Publishing Company, Dordrecht, Holland
About this paper
Cite this paper
Sahade, J. (1969). General Review of Observational Spectroscopic Evidence for Mass Loss in Close Binaries. In: Hack, M. (eds) Mass Loss from Stars. Astrophysics and Space Science Library, vol 13. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-3405-0_19
Download citation
DOI: https://doi.org/10.1007/978-94-010-3405-0_19
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-3407-4
Online ISBN: 978-94-010-3405-0
eBook Packages: Springer Book Archive