Christy, R. F. (1966) Pulsation Theory. Annual Review of Astronomy and Astrophysics, 4 . pp. 353-392. ISSN 0066-4146 http://resolver.caltech.edu/CaltechAUTHORS:20120905-154809533
Full text not available from this repository.
Use this Persistent URL to link to this item: http://resolver.caltech.edu/CaltechAUTHORS:20120905-154809533
Abstract
This review will concentrate on the question of pulsation in what we will call the Cepheid instability strip in the H-R diagram or in the log g-log T_0 diagram. This strip includes, of course, the classical δ Cephei variables, the Population II Cepheids, and the RR Lyrae variables. In addition to these, it appears that the RV Tauri variables, δ Scuti variables, and dwarf Cepheids all belong in this same general class. Clearly excluded from this class are the β Cephei variables, the Mira variables, and other types of red variables. For a more extensive discussion, the review of Ledoux & Walraven (1) is recommended.
| Item Type: | Article | ||||||
|---|---|---|---|---|---|---|---|
| Additional Information: | © 1966 Annual Reviews. The survey of literature for this review was concluded in February 1966. Work supported in part by the National Aeronautics and Space Administration Grant [NsG-426] and the Office of Naval Research Contract [Nonr-220(47)]. | ||||||
| Funders: |
| ||||||
| Record Number: | CaltechAUTHORS:20120905-154809533 | ||||||
| Persistent URL: | http://resolver.caltech.edu/CaltechAUTHORS:20120905-154809533 | ||||||
| Related URLs: | |||||||
| Usage Policy: | No commercial reproduction, distribution, display or performance rights in this work are provided. | ||||||
| ID Code: | 33879 | ||||||
| Collection: | CaltechAUTHORS | ||||||
| Deposited By: | Tony Diaz | ||||||
| Deposited On: | 05 Sep 2012 23:05 | ||||||
| Last Modified: | 05 Sep 2012 23:05 |
Repository Staff Only: item control page
