Astrophysics and Space Science Library: Stellar Pulsation - Nonlinear Studies (Volume 257). Dieser Artikel ist nicht verfügbar.
Sprache: Englisch
Verlag: Kluwer Academic, 2001
Serie: Buch 135 von 228 - Astrophysics and Space Science Library
- Hardcover
- Gebraucht
Anbieter: Anybook.com, Lincoln, Vereinigtes KönigreichAnybook.com
Verkäufer/-in mit 5 Sternen
AbeBooks-Verkäufer/-in seit 22. Dezember 1999
Nicht verfügbar
Hardcover
Zustand: Gebraucht - Befriedigend
EUR 17,18
Artikelbeschreibung vom Verkäufer
Volume 257. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In good all round condition. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,650grams, ISBN:9780792368182.
Bestandsnummer des Verkäufers 8697609
- Titel
- Astrophysics and Space Science Library: Stellar Pulsation - Nonlinear Studies (Volume 257)
- Autor
- Takeuti, M. (ed) et al
- Verlag
- Kluwer Academic
- Veröffentlichungsjahr
- 2001
- Zustand
- Good
- Einband
- Hardcover
- Sprache
- Englisch
- ISBN-10
- 0792368185
- ISBN-13
- 9780792368182
- Artikelgewicht
- 650 Gramm
- Serie
- Buch 135 von 228: Astrophysics and Space Science Library
- Verkäuferkataloge
- Astronomy & Cosmology
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.
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.
„Inhaltsangabe“ gehört möglicherweise zu einer anderen Auflage dieses Titels.