Radial Velocity Measurements of Twenty-One Long-Period Variable Stars

1965 ◽  
Vol 77 ◽  
pp. 214 ◽  
Author(s):  
Charles L. Perry ◽  
William P. Bidelman
1979 ◽  
Vol 46 ◽  
pp. 199-213
Author(s):  
L. A. Willson

The first part of this paper contains a synthesis of the results of numerical and analytical theoretical models for the velocity structure of the atmospheres of the long period variable stars (LPVs). The details of these derivations have been presented elsewhere (Willson and Hill 1978; Hill and Willson 1978). The discussion of the models in this paper is therefore limited to summarizing the earlier results in a form appropriate to the interpretation of observed velocities. In the second part of the paper the methods described in the first part are applied to five stars with periods ranging from 150dto 407d, and masses and radii are derived from velocity information for each of these stars. In the third section a general mass-radius relationship for the long period variable stars is derived from these points and compared to independent observational constraints.


1989 ◽  
Vol 106 ◽  
pp. 241-257
Author(s):  
T. Lloyd Evans

The study of long period variable stars has been transformed in recent years by two observational developments. Large samples of stars have been observed at infrared wavelengths, providing knowledge of the intrinsic properties of the star as well as of circumstellar dust shells, and these observations have been extended to the variables in well defined stellar systems to allow their properties to be studied in relation to the stellar population to which they belong. Spectroscopic determinations of chemical composition have also provided several crucial insights.


2018 ◽  
Vol 156 (1) ◽  
pp. 15 ◽  
Author(s):  
L. D. Matthews ◽  
M. J. Reid ◽  
K. M. Menten ◽  
K. Akiyama

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