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Titlebook: Binary Stars: Selected Topics on Observations and Physical Processes; Lectures Held at the F. Carlos Lázaro,Maria J. Arévalo Book 2001 Spri

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樓主: Falter
21#
發(fā)表于 2025-3-25 07:11:19 | 只看該作者
Michael Buschhüter,Andreas Striegelmake no attempt to be comprehensive in my coverage. The reader is referred to Brian Warner’s book [.] for such a treatment of cataclysmic variable stars. The theory behind the accretion discs which play such a key r?le in these objects is covered elsewhere in this volume by J.Smak.
22#
發(fā)表于 2025-3-25 07:59:08 | 只看該作者
Observations of Cataclysmic Variable and Double Degenerate Stars,make no attempt to be comprehensive in my coverage. The reader is referred to Brian Warner’s book [.] for such a treatment of cataclysmic variable stars. The theory behind the accretion discs which play such a key r?le in these objects is covered elsewhere in this volume by J.Smak.
23#
發(fā)表于 2025-3-25 14:07:47 | 只看該作者
24#
發(fā)表于 2025-3-25 18:47:00 | 只看該作者
https://doi.org/10.1007/978-3-8349-8060-1tellar rotation and the quest to understand stellar magnetic activity is thus always a quest to understand stellar rotation. In this lecture, we will focus on the many aspects of stellar rotation and compare the situation of binary stars with their single star counterparts whenever appropriate. I wi
25#
發(fā)表于 2025-3-25 23:22:12 | 只看該作者
Konzeptionelle Grundlagen der IFRS,ded to the whole Galaxy. Before starting the study of evolution of close binary systems, we examine rst the evolution of single stars. So we begin to deal with the stellar structure processes, stellar evolution in general, we investigate how evolution occurs dierently for stars of low, intermediate
26#
發(fā)表于 2025-3-26 02:19:17 | 只看該作者
Magnetic Activity in Binary Stars,tellar rotation and the quest to understand stellar magnetic activity is thus always a quest to understand stellar rotation. In this lecture, we will focus on the many aspects of stellar rotation and compare the situation of binary stars with their single star counterparts whenever appropriate. I wi
27#
發(fā)表于 2025-3-26 05:00:24 | 只看該作者
28#
發(fā)表于 2025-3-26 11:30:23 | 只看該作者
29#
發(fā)表于 2025-3-26 13:20:57 | 只看該作者
Magnetic Activity in Binary Stars,r star is in a state of sunspot minimum or maximum, respectively. More physically, we mean with activity all phenomena inside and outside of a star that are related to its magnetic field, e.g. the rise of flux tubes in a stellar convection zone and their appearance as spots and plages on the stellar
30#
發(fā)表于 2025-3-26 19:20:16 | 只看該作者
Observations of Cataclysmic Variable and Double Degenerate Stars,heir evolution, but in this case also because they are personal interests of mine. The detailed topics that I discuss are also personal choices and I make no attempt to be comprehensive in my coverage. The reader is referred to Brian Warner’s book [.] for such a treatment of cataclysmic variable sta
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