The History and Development of Nonlinear Stellar Pulsation Codes

The History and Development of Nonlinear Stellar Pulsation Codes
Author:
Publisher:
Total Pages:
Release: 1987
Genre:
ISBN:

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This review is limited to the history and development of nonlinear stellar pulsation codes and methods. The narrative includes examples of practical interest in the application of these numerical methods to problems in stellar pulsation such as Cepheid mass discrepancy, the delineation of the RR Lyrae instability strip, and the question of the development of double-mode pulsation as observed in Cepheids, RR Lyrae and other variable stars. 15 refs.

Stellar Pulsation - Nonlinear Studies

Stellar Pulsation - Nonlinear Studies
Author: Mine Takeuti
Publisher: Springer Science & Business Media
Total Pages: 237
Release: 2013-03-09
Genre: Science
ISBN: 9401596980

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Stellar pulsations provide a complex system in stars. This complexity is studied by analyzing the non-sinusoidal, semi-regular, or irregular light curves. This unique volume summarizes the application of recent theoretical results obtained from stellar pulsation studies. In addition, the latest developments in hydrodynamic simulations are discussed. A historical sketch of the study of beat Cepheids, first known for their variable amplitudes, is given as an introduction to the book. This introduction clearly demonstrates how complicated the study of variable stars can be, and therefore challenges and invites the reader to study the entire book.

Literature 1989, Part 1

Literature 1989, Part 1
Author: Astronomisches Rechen-Institut
Publisher: Springer Science & Business Media
Total Pages: 1433
Release: 2013-11-11
Genre: Science
ISBN: 3662123703

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From the reviews: "Astronomy and Astrophysics Abstracts has appeared in semi-annual volumes since 1969 and it has already become one of the fundemental publications in the fields of astronomy, astrophysics and neighbouring sciences. It is the most important English-language abstracting journal in the mentioned branches. ...The abstracts are classified under more than a hundred subject categories, thus permitting a quick survey of the whole extended material. The AAA is a valuable and important publication for all students and scientists working in the fields of astronomy and related sciences. As such it represents a necessary ingredient of any astronomical library all over the world." Space Science Review# "Dividing the whole field plus related subjects into 108 categories, each work is numbered and most are accompanied by brief abstracts. Fairly comprehensive cross-referencing links relevant papers to more than one category, and exhaustive author and subject indices are to be found at the back, making the catalogues easy to use. The series appears to be so complete in its coverage and always less than a year out of date that I shall certainly have to make a little more space on those shelves for future volumes." The Observatory Magazine#

Multimode Stellar Pulsations

Multimode Stellar Pulsations
Author: Géza Kovács
Publisher:
Total Pages: 324
Release: 1988
Genre: Pulsating stars
ISBN:

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Stellar Pulsation - Nonlinear Studies

Stellar Pulsation - Nonlinear Studies
Author: Mine Takeuti
Publisher: Springer
Total Pages: 0
Release: 2010-12-05
Genre: Science
ISBN: 9789048156535

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Stellar pulsations provide a complex system in stars. This complexity is studied by analyzing the non-sinusoidal, semi-regular, or irregular light curves. This unique volume summarizes the application of recent theoretical results obtained from stellar pulsation studies. In addition, the latest developments in hydrodynamic simulations are discussed. A historical sketch of the study of beat Cepheids, first known for their variable amplitudes, is given as an introduction to the book. This introduction clearly demonstrates how complicated the study of variable stars can be, and therefore challenges and invites the reader to study the entire book.

Energy Research Abstracts

Energy Research Abstracts
Author:
Publisher:
Total Pages: 664
Release: 1989
Genre: Power resources
ISBN:

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