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Titlebook: Stellar Astrophysics; A Tribute to Helmut K. S. Cheng,K. C. Leung,T. P. Li Conference proceedings 2003 Springer Science+Business Media Dor

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發(fā)表于 2025-3-21 17:52:12 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Stellar Astrophysics
副標(biāo)題A Tribute to Helmut
編輯K. S. Cheng,K. C. Leung,T. P. Li
視頻videohttp://file.papertrans.cn/878/877147/877147.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Stellar Astrophysics; A Tribute to Helmut  K. S. Cheng,K. C. Leung,T. P. Li Conference proceedings 2003 Springer Science+Business Media Dor
描述The Pacific Rim Conferences for the first decade from the mid 1980‘s to the mid 1990‘s were primary concerned with binary stars research. The Conference expanded to all areas of Stellar Astrophysics for the last two meetings in Hong Kong; at Hong Kong University of Science and Technology in 1997 and at the Hong Kong University in 1999. At the conclusion of the very successful Pacific Rim Conference on Stellar Astrophysics held in Hong Kong University, members of the Sci- entific Organizing Committee began planning for the next conference. We approached Professor Tan Lu of Nanjing University and Professor Tipei Li of the Institute of High Energy Physics about hosting a con- ference in China. The city of Xi‘a(chǎn)n in Shaanxi province and a city in Yunnan province, were considered to be the most likely locations. It be- came crucial to find the right person to serve as Chair (or Co-chairs) for the Local Organizing Committee. Initially, Professor Lu was the logical choice but he declined for personal reasons. Professor Li was invited to lead a new department of Astrophysics at Tsinghua University so he could not take on the additional load of chairing the LOC. Professor Gang Zhao of Beijin
出版日期Conference proceedings 2003
關(guān)鍵詞astronomy; astrophysics; star; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-017-0403-8
isbn_softcover978-90-481-6452-3
isbn_ebook978-94-017-0403-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 2003
The information of publication is updating

書目名稱Stellar Astrophysics影響因子(影響力)




書目名稱Stellar Astrophysics影響因子(影響力)學(xué)科排名




書目名稱Stellar Astrophysics網(wǎng)絡(luò)公開度




書目名稱Stellar Astrophysics網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Stellar Astrophysics被引頻次




書目名稱Stellar Astrophysics被引頻次學(xué)科排名




書目名稱Stellar Astrophysics年度引用




書目名稱Stellar Astrophysics年度引用學(xué)科排名




書目名稱Stellar Astrophysics讀者反饋




書目名稱Stellar Astrophysics讀者反饋學(xué)科排名




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Gamma-Ray Pulsars in Gould Belt and Unidentified Gamma-Ray Sources in Medium Latitudes can exist even their age > 10. yr old. We use Monte Carlo techniques to simulate the statistical properties of rotation-powered pulsars in the Gould Belt. If the pulsar birth rate in Gould Belt is 3 × 10..., the gamma-ray pulsars in this region, which can be detected by EGRET, will must be dominate
板凳
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Magnetars and Pulsars: A Missing Link fields, i.e., magnetars, marking them a distinguished species from the conventional species of spindown-powered isolated neutron stars, i.e., radio pulsars. The current arguments in favor of the magnetar interpretation of SGR/AXP phenomenology will be outlined, and the two energy sources in magneta
地板
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Phase Transition in Rotating Hybrid Starsmoment of inertia, and even results in an era of spin-up of the pulsar (Glendenning, Pei, & Weber 1997, hereafter GPW) . We have found that the equation of states of the crust of neutron star and the accuracy of the numerical models which can be used to determinate the stellar rotating properties ar
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發(fā)表于 2025-3-23 03:06:55 | 只看該作者
Accretion Disk Oscillations and QPOs in X-Ray Binariesation modes in a relativistic accretion disk. Here we studied the non-damping feature of some oscillation modes by considering the radial perturbations and viscosity effects. We found that the non-damping fundamental modes can be amplified significantly in the inner disk when the viscosity parameter
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發(fā)表于 2025-3-23 09:29:32 | 只看該作者
Bare Strange Quark Stars: Formation and Emissionmperature after the supernova detonation flame, and a crust can also hardly form except for a super-Eddington accretion. The magnetosphere of a bare strange star is composed mainly of e. pair plasma, where both inner and outer vacuum gaps work for radio as well as high energy nonthermal emission. A
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