Abstract
We describe a simple model for the calculation of the flow velocity in the envelopes of M-type Mira variables. The results are compared with the observed diagram of terminal velocity versus period.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Bedijn, P.: 1977, Ph.D. thesis, Leiden University.
Dickinson, D.F. and Chaisson, E.J.: 1973, Astrophys. J. 181, L135.
Jones, T.W. and Merrill, K.M.: 1976, Astrophys. J. 209, 509.
Kwok, S.: 1975, Astrophys. J. 198, 583.
Salpeter, E.E.: 1974, Astrophys. J. 193, 585.
Winnberg, A.: 1977, I.A.U. Colloquium No. 42 (Bamberg), p. 495.
Wood, P.R. and Cahn, J.H.: 1977, Astrophys. J. 211, 499.
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1981 D. Reidel Publishing Company
About this paper
Cite this paper
Olnon, F.M. (1981). The Expansion Velocities in Mira Envelopes. In: Iben, I., Renzini, A. (eds) Physical Processes in Red Giants. Astrophysics and Space Science Library, vol 88. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-8492-9_24
Download citation
DOI: https://doi.org/10.1007/978-94-009-8492-9_24
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-009-8494-3
Online ISBN: 978-94-009-8492-9
eBook Packages: Springer Book Archive