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Titlebook: Activity in Red-Dwarf Stars; Proceedings of the 7 Patrick B. Byrne,Marcello Rodonò Conference proceedings 1983 Springer Science+Business Me

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發(fā)表于 2025-3-21 16:29:35 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
期刊全稱Activity in Red-Dwarf Stars
期刊簡(jiǎn)稱Proceedings of the 7
影響因子2023Patrick B. Byrne,Marcello Rodonò
視頻videohttp://file.papertrans.cn/145/144311/144311.mp4
學(xué)科分類Astrophysics and Space Science Library
圖書封面Titlebook: Activity in Red-Dwarf Stars; Proceedings of the 7 Patrick B. Byrne,Marcello Rodonò Conference proceedings 1983 Springer Science+Business Me
影響因子IAU Colloquium No. 71 had its immediate origins in a small gathering of people interested. in the optical and UV study of flare stars which took place during the 1979 Montreal General Assembly. We recognized that a fundamental change was taking place in the study of these objects. Space-borne instruments (especially lUE and Einstein) and a new genera- tion of ground-based equipment were having a profound effect on the range of investigations it was possible to make. To extract maximum benefit from these new possibilities it would be necessary as never before to have good communication with colleagues in other disciplines, for instance,. with atomic and solar physicists. Similarly, studies of phenomena associated with the outer atmospheres of the late-type stars could now hope to give significant insights into certain aspects of solar activity. So, in view of the wide range of backgrounds of those participating, the meeting had an unusually high proportion of invited reviews while most of the contributed papers were presented as posters. It is gratifying that in the short time since the meeting a good deal of correspondence has been received from participants remarking on the succes
Pindex Conference proceedings 1983
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Global and Photospheric Physical Parameters of Active Dwarf Starstungsweise) der Disziplin sowie der Abgrenzung gegenüber anderen Wissenschaften kann man sinnvollerweise erst dann sprechen, wenn hinsichtlich der Frage ?reine oder angewandte Wissenschaft” Einigkeit besteht., was nicht selten übersehen wird.. Bevor wir indessen auf den Unterschied zwischen ?reinen“
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The Structure and Energy Balance in Main Sequence Starsbe severely trimmed and skimmed to fit “neatly” into the selected concepts. As local researchers provide evidence that what was found in the West is also to be found in an Asian context, the universalizing claim of Western concepts is (re-)affirmed. Both processes are unhappy ones, even if there wer
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Late-Type Ca II Emission-Line Stars in the Southern Hemisphere invited speakers. The aim was to get the participants aware of the current state of the art and to highlight the main outstanding issues. The second day consisted of the Workshop participants splitting into three groups and discussing specific issues in depth. Plenary sessions helped to keep the individual g978-3-642-70921-0978-3-642-70919-7
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Some Properties of Stellar Transition Regions, status of the big cat remains precarious. Rigorous monitoring of surviving wild tiger populations continues to be essential for both understanding and recovering wild tigers. However, many tiger monitoring programs lack the necessary rigor to generate the reliable results. While the deployment of
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Quiescent Coronae of Active Chromosphere Starsne metabolism, uric acid. Thus it has been proposed that a potent inhibitor of PNP might serve as a biochemical modifier in chemotherapy with purine nucleoside analogs, as a selective immunosuppressive agent, and perhaps in the treatment of secondary gout (Parks .., 1981; Stoeckler .., 1980a, 1982;
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Einstein and IUE Observations of Nearby Red Dwarfsfor a proper literature appraisal.. Addressing that gap, this book discusses more practical aspects of clinical research and biostatistics in oncology, instead of relying only on mathematical formulas and theoretical considerations. Methods and Biostatistics in Oncology will help readers develop the
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