標(biāo)題: Titlebook: Binary Stars: Selected Topics on Observations and Physical Processes; Lectures Held at the F. Carlos Lázaro,Maria J. Arévalo Book 2001 Spri [打印本頁] 作者: Falter 時間: 2025-3-21 18:27
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作者: gangrene 時間: 2025-3-21 22:23 作者: prolate 時間: 2025-3-22 03:42
Binary Stars: Selected Topics on Observations and Physical Processes978-3-540-44395-7Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: Polydipsia 時間: 2025-3-22 08:36
Konzeptionelle Grundlagen der IFRS,Topics covered by this review are: observational data, basic parameters and standard model for non-magnetic cataclysmic variables (CV’s), structure of accretion disks in CV’s and their thermal instability, dwarf nova outbursts, boundary layer, and origin of emission lines.作者: 思鄉(xiāng)病 時間: 2025-3-22 10:07
Cataclysmic Variables,Topics covered by this review are: observational data, basic parameters and standard model for non-magnetic cataclysmic variables (CV’s), structure of accretion disks in CV’s and their thermal instability, dwarf nova outbursts, boundary layer, and origin of emission lines.作者: GENRE 時間: 2025-3-22 15:23
Book 2001volution. The six lectures in this book give both a readable introduction and an up-to-date review of nearly all aspects of? research into binary stars, including the range from common binaries to more exotic systems composed of white dwarfs, neutron stars and black holes.作者: avarice 時間: 2025-3-22 19:33
F. Carlos Lázaro,Maria J. ArévaloIncludes supplementary material: 作者: murmur 時間: 2025-3-22 21:43
Lecture Notes in Physicshttp://image.papertrans.cn/b/image/186285.jpg作者: arcane 時間: 2025-3-23 03:43 作者: 生意行為 時間: 2025-3-23 05:49
https://doi.org/10.1007/978-3-8349-8060-1r 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作者: Peak-Bone-Mass 時間: 2025-3-23 12:16 作者: 禍害隱伏 時間: 2025-3-23 15:07
Konzeptionelle Grundlagen der IFRS,ars are born. Stars can be born as singles, in pairs, or in multiple systems. A large fraction of the stars belongs to binary systems. Hence it is essential to know how stellar masses are distributed at birth, how many stars are formed, not only as singles, but also what fraction originates as binar作者: 背帶 時間: 2025-3-23 20:19
https://doi.org/10.1007/978-3-8349-8060-1nts. The latter provide the most compelling evidence for the existence of black holes in the Universe, with nine well-established dynamical studies. We review the techniques employed to extract the component masses and discuss the importance of systematic eects. Despite the growing number of black h作者: LINE 時間: 2025-3-24 00:07 作者: 武器 時間: 2025-3-24 06:24 作者: insomnia 時間: 2025-3-24 08:39 作者: LATHE 時間: 2025-3-24 14:42
0075-8450 y all aspects of? research into binary stars, including the range from common binaries to more exotic systems composed of white dwarfs, neutron stars and black holes.978-3-642-07455-4978-3-540-44395-7Series ISSN 0075-8450 Series E-ISSN 1616-6361 作者: 小淡水魚 時間: 2025-3-24 18:36 作者: Memorial 時間: 2025-3-24 22:47 作者: CHIDE 時間: 2025-3-25 01:50 作者: 粗糙 時間: 2025-3-25 07:11
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.作者: 子女 時間: 2025-3-25 07:59
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.作者: interpose 時間: 2025-3-25 14:07 作者: 同時發(fā)生 時間: 2025-3-25 18:47
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作者: meritorious 時間: 2025-3-25 23:22
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 作者: Protein 時間: 2025-3-26 02:19
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作者: 懸掛 時間: 2025-3-26 05:00 作者: Allure 時間: 2025-3-26 11:30 作者: 學(xué)術(shù)討論會 時間: 2025-3-26 13:20
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作者: CHOKE 時間: 2025-3-26 19:20
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作者: 信徒 時間: 2025-3-26 22:24 作者: coltish 時間: 2025-3-27 01:48 作者: Esophagus 時間: 2025-3-27 07:54 作者: 原告 時間: 2025-3-27 12:24 作者: 聚集 時間: 2025-3-27 15:01
Peter K?hler,Ralf Hoffmann,Martina K?hlerpolicy in the "acquis communautaire". European competition policy is now at a tuming turning point in its history. In May 2004, ten countries will join a new European Union composed of twenty-five Member States and 450 million people. This massive accession to the EU is of paramount importance to th作者: 投票 時間: 2025-3-27 18:22
