標(biāo)題: Titlebook: Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems; A. H. Batten Book 1973 International Astronomical Union 197 [打印本頁(yè)] 作者: Definite 時(shí)間: 2025-3-21 17:45
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems影響因子(影響力)
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems影響因子(影響力)學(xué)科排名
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems網(wǎng)絡(luò)公開(kāi)度
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems網(wǎng)絡(luò)公開(kāi)度學(xué)科排名
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems被引頻次
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems被引頻次學(xué)科排名
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems年度引用
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems年度引用學(xué)科排名
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems讀者反饋
書(shū)目名稱Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems讀者反饋學(xué)科排名
作者: languid 時(shí)間: 2025-3-21 21:10 作者: 初次登臺(tái) 時(shí)間: 2025-3-22 01:33 作者: insert 時(shí)間: 2025-3-22 08:33 作者: sigmoid-colon 時(shí)間: 2025-3-22 09:25
Book 1973Plavec. In addition, J. Sahade and F. B. Wood acted as advisory members. Local organization was entrusted to a committee consisting of A. H. Batten, E. K. Lee, and C. D. Scarfe. The final dates selected were September 6-12, 1972, and the Sym- posium was held at the Island Hall Hotel, Parksville, B. 作者: PSA-velocity 時(shí)間: 2025-3-22 14:30 作者: PSA-velocity 時(shí)間: 2025-3-22 19:19 作者: 調(diào)味品 時(shí)間: 2025-3-23 00:41 作者: LVAD360 時(shí)間: 2025-3-23 04:02 作者: SPURN 時(shí)間: 2025-3-23 09:26
Evolutionary Aspects of Circumstellar Matter in Binary Systems,of the helium main sequence, while the other component may be a rather inactive main-sequence star. Some shell stars may be products of mass transfer. Mass loss from convective envelopes is also discussed..Loss of mass and of angular momentum from many binary systems must be anticipated. Behavior of作者: 高談闊論 時(shí)間: 2025-3-23 11:38
Summary,been present at this meeting and realize how many astronomers are now interested, strongly interested, in the field of close binaries and how much the field has and is expanding taking also up the efforts of researchers that work in the radio and X-ray regions and attracting the attention of those w作者: 種子 時(shí)間: 2025-3-23 16:28 作者: 寬大 時(shí)間: 2025-3-23 21:16 作者: 放縱 時(shí)間: 2025-3-23 22:36
978-90-277-0362-0International Astronomical Union 1973作者: companion 時(shí)間: 2025-3-24 06:03
Extended Atmospheres and Circumstellar Matter in Spectroscopic Binary Systems978-94-010-2614-7Series ISSN 1743-9213 Series E-ISSN 2352-2186 作者: enlist 時(shí)間: 2025-3-24 08:39
J.-L. Touraine,M. C. Favrot,M. El Ansary establishing limiting values that could be useful in any theoretical treatment of circumstellar structure. Densities of the order of 10. particles cm. are found for streams and disks, although there is evidence for regions of much lower density in many systems, and some systems may have much denser作者: charisma 時(shí)間: 2025-3-24 14:12 作者: 出汗 時(shí)間: 2025-3-24 17:52
https://doi.org/10.1007/978-3-031-50844-8ll stars and Be stars are considered together, the observed differences between them being considered as due to the size of the envelope and the angle that the rotational axis makes with the line of sight. Rotational ejection of matter is insufficient to account for the formation of the envelopes. T作者: nonsensical 時(shí)間: 2025-3-24 22:23 作者: Ascendancy 時(shí)間: 2025-3-25 01:25
Immunopathology of Immune Complex Disease,nd discuss critically the present status of the theory of three types of extended atmospheres (i.e. atmospheres in which the average photon mean-free-path is the same order of magnitude or larger than the stellar radius):.In (1) we study the importance of the ‘forward peaking’ of the radiation field作者: 我沒(méi)有命令 時(shí)間: 2025-3-25 07:12
https://doi.org/10.1007/978-4-431-55726-5ss loss in the past: Algol-like semidetached binaries, some shell stars (AX Mon), some binary X-ray sources (Cen X-3, Her X-l), the recurrent nova T CrB, helium-rich binaries . Sgr and KS Per, and the symbiotic variables..Algol-like binaries like U Sge cannot be products of a conservative case A of 作者: Allege 時(shí)間: 2025-3-25 09:01
John W. Hadden,Ronald G. Coffeyouched upon many items, some of them apparently not strictly connected with the subject of the meeting but helpful to clarify the picture related to close binaries and aimed at establishing differences with single stars, whenever possible. Therefore, my task would be somewhat difficult it if were no作者: violate 時(shí)間: 2025-3-25 12:56 作者: 胡言亂語(yǔ) 時(shí)間: 2025-3-25 15:56
Expanding Envelopes of Stars,se is complicated by the known binary nature of many Wolf-Rayet stars. Other groups of stars possessing envelope-like structures — U Gem stars and old novae, symbiotic stars, and T Tauri stars — are briefly mentioned. The problems of stellar envelopes, first listed by Struve thirty years ago, are still unsolved.作者: 敏捷 時(shí)間: 2025-3-25 23:17
Book 1973 Observatory to the Executive Committee of the International Astronomical Union in the summer of 1969. It received the support of the presidents of Commissions 29 (Stellar Spectra), 30 (Radial Velocities), 36 (Stellar Atmospheres), and 42 (Photometric Double Stars). Approval in principle was given b作者: 赦免 時(shí)間: 2025-3-26 01:56 作者: Projection 時(shí)間: 2025-3-26 04:23 作者: 暗指 時(shí)間: 2025-3-26 10:25
Immunopathology of Immune Complex Disease,es by the action of the radiation force..In (3) the large differences in the coronal properties of stars of different chemical composition are emphasized. We draw attention to the partially unexplored but probably very interesting properties of coronae of helium-rich stars.作者: MAOIS 時(shí)間: 2025-3-26 15:12
Problems of Gaseous Motion Around Stars,ng and the orbital period is discussed. The relation of circumstellar streams to period changes is mentioned. Finally, the influence of magnetic fields on the circumstellar material and the system is discussed.作者: 擴(kuò)張 時(shí)間: 2025-3-26 20:33 作者: dilute 時(shí)間: 2025-3-26 21:32 作者: Debrief 時(shí)間: 2025-3-27 01:21 作者: resilience 時(shí)間: 2025-3-27 06:05 作者: DENT 時(shí)間: 2025-3-27 09:32 作者: 緯度 時(shí)間: 2025-3-27 14:43 作者: ODIUM 時(shí)間: 2025-3-27 17:53 作者: Arthropathy 時(shí)間: 2025-3-27 23:22
Summary,ouched upon many items, some of them apparently not strictly connected with the subject of the meeting but helpful to clarify the picture related to close binaries and aimed at establishing differences with single stars, whenever possible. Therefore, my task would be somewhat difficult it if were no作者: 弄皺 時(shí)間: 2025-3-28 05:47
Jerome Friedmank to the basics—an application of microeconomics to biofuels production and consumption, the price and quantity links backwards to the feedstocks and forward to energy and crude oil markets, with due regard to co-products, joint products and by-products along the way. We simply assume profit-maximizing agents under competition.作者: Horizon 時(shí)間: 2025-3-28 08:29 作者: MIME 時(shí)間: 2025-3-28 11:41
K. M. Guglielmi,E. M. Johnson,T. Stehle,T. S. Dermody. Because of the advantages of flexible start-stop flexibility, quick response, and pollution-free characteristic, hydropower could effectively complement the local consumption of wind and photovoltaic generation. A capacity allocation method that aims at minimizing the investment cost of pumped sto作者: 我的巨大 時(shí)間: 2025-3-28 15:19
nnection with lived experience might be established.Presents.This book draws on existential theory and original research to present the conceptual framework for an understanding of existential authenticity and demonstrates how this approach might be adopted in practice. The authors explore how a non
