標(biāo)題: Titlebook: Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems; Thomas B. Ake,Elizabeth Griffin Book 2015 Springer International Publishi [打印本頁] 作者: Grievous 時間: 2025-3-21 19:59
書目名稱Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems影響因子(影響力)
書目名稱Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems影響因子(影響力)學(xué)科排名
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書目名稱Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems被引頻次
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書目名稱Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems讀者反饋
書目名稱Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems讀者反饋學(xué)科排名
作者: hidebound 時間: 2025-3-21 22:26
Living reference work 20200th editionon of winds in single cool, evolved stars and in eclipsing binary stars, including physical models that have recently been proposed. It describes the successes that have been achieved so far by invoking acoustic and MHD waves to provide a physical description of plasma heating and wind acceleration, and discusses the challenges that still remain.作者: NAIVE 時間: 2025-3-22 04:22
Katrin M?ltgen-Sicking,Nicole Najemnikellar disks is helping to solve long-standing problems related to carbon stars, and summarizes some of the state-of-the-art techniques that are now being used to image spots and convective cells on supergiants.作者: isotope 時間: 2025-3-22 06:24
Atmospheric Heating and Wind Acceleration in Cool Evolved Stars,on of winds in single cool, evolved stars and in eclipsing binary stars, including physical models that have recently been proposed. It describes the successes that have been achieved so far by invoking acoustic and MHD waves to provide a physical description of plasma heating and wind acceleration, and discusses the challenges that still remain.作者: 浮雕 時間: 2025-3-22 10:36
Optical Interferometry of Giants and Supergiants,ellar disks is helping to solve long-standing problems related to carbon stars, and summarizes some of the state-of-the-art techniques that are now being used to image spots and convective cells on supergiants.作者: Epithelium 時間: 2025-3-22 14:17 作者: Epithelium 時間: 2025-3-22 19:53 作者: 美學(xué) 時間: 2025-3-22 22:41
https://doi.org/10.1007/978-3-658-36629-2 the framework of modern observing, data management and computing, outlines the principal features of the chromospheric-eclipse phenomena which single out the .?Aur?binaries for special study, and describes the considerable potential which this remarkable yet very select group of stars offers for increasing our understanding of stellar physics.作者: BIAS 時間: 2025-3-23 02:02 作者: 吼叫 時間: 2025-3-23 05:38 作者: 大笑 時間: 2025-3-23 13:44 作者: FISC 時間: 2025-3-23 15:23
Tanja Klenk,Frank Nullmeier,G?ttrik Wewerthe system and components, a high-mass versus low-mass model dilemma persists. This chapter examines some of the recent developments and attempts to place the system among the pantheon of binary types. It also offers suggestions for observational tests prior to the next eclipse in 2037.作者: 熄滅 時間: 2025-3-23 19:53 作者: 施加 時間: 2025-3-24 00:28
, Aurigae: A Two Century Long Dilemma Persists,the system and components, a high-mass versus low-mass model dilemma persists. This chapter examines some of the recent developments and attempts to place the system among the pantheon of binary types. It also offers suggestions for observational tests prior to the next eclipse in 2037.作者: maudtin 時間: 2025-3-24 05:30 作者: 子女 時間: 2025-3-24 07:38
Achim Kie?ig,Katja Lohmann,Cornelia Zanger data that have been used in those analyses, and examines each of the 10 known eclipsing systems in turn, except for VV?Cep which is treated separately in Chap.?. It describes what has been achieved by modelling, and assesses what has been learned so far about the mass loss and winds from the cool g作者: 按時間順序 時間: 2025-3-24 13:19
Handbuch Digitaler Schnittstellension to what can be learned by eclipse mapping, but are fraught with many challenges. The space-UV absorption spectrum is extremely rich, and line blending is severe. Wind interaction and accretion effects are prominent, and the spectrum of the B star companion is heavily veiled by overlying Balmer 作者: extinct 時間: 2025-3-24 17:46 作者: Insul島 時間: 2025-3-24 22:09
Living reference work 20200th edition, show extended and highly turbulent chromospheres, which develop into slow massive winds. The associated continuous mass loss has a significant impact on stellar evolution, and thence on the chemical evolution of galaxies. Yet despite the fundamental importance of those winds in astrophysics, the q作者: largesse 時間: 2025-3-24 23:15 作者: 露天歷史劇 時間: 2025-3-25 07:15 作者: Hemiparesis 時間: 2025-3-25 10:19
The , Aurigae Binaries, Dominion Astrophysical Observatory, and his contemporaries further afield, achieved during the era of pre-electronic data. It places the topic within the framework of modern observing, data management and computing, outlines the principal features of the chromospheric-eclipse phenomena which single作者: 南極 時間: 2025-3-25 12:21 作者: Accommodation 時間: 2025-3-25 17:01 作者: Substance-Abuse 時間: 2025-3-25 22:35
, Aurigae: A Two Century Long Dilemma Persists,eclipse, 2009-2011, was monitored with an array of new and old astronomical techniques, leading to new evidence concerning the nature of the eclipsing body and its contents. While this has led to new insights about the state of the F superigant star and to more clues about the evolutionary state of 作者: 重力 時間: 2025-3-26 01:35 作者: 的是兄弟 時間: 2025-3-26 08:22 作者: 無能力 時間: 2025-3-26 12:01 作者: 業(yè)余愛好者 時間: 2025-3-26 16:14 作者: jovial 時間: 2025-3-26 20:25
Handbuch Digitaler Schnittstellenthe whole extended chromosphere of the M supergiant. Spectrum formation in the atmosphere of VV Cep is more complex than in the other . Aur binaries owing to the much higher rate of mass loss from the primary. This chapter summarizes the fundamental stellar and orbit parameters of VV Cep, and presen作者: 進(jìn)步 時間: 2025-3-27 01:00 作者: interior 時間: 2025-3-27 05:07 作者: 貝雷帽 時間: 2025-3-27 06:38
The Special Case of VV Cephei,the whole extended chromosphere of the M supergiant. Spectrum formation in the atmosphere of VV Cep is more complex than in the other . Aur binaries owing to the much higher rate of mass loss from the primary. This chapter summarizes the fundamental stellar and orbit parameters of VV Cep, and presen作者: 暫時休息 時間: 2025-3-27 12:33 作者: 禍害隱伏 時間: 2025-3-27 14:20 作者: guardianship 時間: 2025-3-27 19:02
978-3-319-35676-1Springer International Publishing Switzerland 2015作者: 終端 時間: 2025-3-27 23:57
Giants of Eclipse: The ζ Aurigae Stars and Other Binary Systems978-3-319-09198-3Series ISSN 0067-0057 Series E-ISSN 2214-7985 作者: 珊瑚 時間: 2025-3-28 05:33
Nonmultiplying Bacteria are Profoundly Tolerant to Antibiotics,ng sensitive organisms. For this reason, a prolonged length of chemotherapy, lasting 6 months, is necessary to achieve cure. This long duration of treatment is due to the slow, inadequate effect of antibiotics on nonmultiplying persistent bacteria. Similar problems with eradication of persistent bac作者: miscreant 時間: 2025-3-28 09:18 作者: certitude 時間: 2025-3-28 11:17 作者: Tracheotomy 時間: 2025-3-28 14:38 作者: CLOUT 時間: 2025-3-28 19:28
