標(biāo)題: Titlebook: Instabilities in Luminous Early Type Stars; Proceedings of a Wor Henny J. G. L. M. Lamers,Camiel W. H. Loore Conference proceedings 1987 D. [打印本頁] 作者: lexicographer 時(shí)間: 2025-3-21 18:30
書目名稱Instabilities in Luminous Early Type Stars影響因子(影響力)
書目名稱Instabilities in Luminous Early Type Stars影響因子(影響力)學(xué)科排名
書目名稱Instabilities in Luminous Early Type Stars網(wǎng)絡(luò)公開度
書目名稱Instabilities in Luminous Early Type Stars網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Instabilities in Luminous Early Type Stars被引頻次
書目名稱Instabilities in Luminous Early Type Stars被引頻次學(xué)科排名
書目名稱Instabilities in Luminous Early Type Stars年度引用
書目名稱Instabilities in Luminous Early Type Stars年度引用學(xué)科排名
書目名稱Instabilities in Luminous Early Type Stars讀者反饋
書目名稱Instabilities in Luminous Early Type Stars讀者反饋學(xué)科排名
作者: 供過于求 時(shí)間: 2025-3-21 20:29
Giant Outbursts of the Eta Carinae - P Cygni TypeDuring such an event, the mass loss rate can be of the order of 0.1 M? yr. for several years. We do not yet understand this phenomenon, partly because most relevant theoretical work has been devoted instead to more familiar, less dramatic stellar winds.作者: Heterodoxy 時(shí)間: 2025-3-22 02:57
Radiation Driven Instabilitiescur in the supersonic parts of the winds, where as many as one hundred e-folds of linear growth can occur during a typical outflow time. The nonlinear growth of such instabilities can possibly account for the observed superionization and X-ray emission in these stars. Developments in the linear theory of these instabilities is reviewed.作者: epinephrine 時(shí)間: 2025-3-22 05:57 作者: Arteriography 時(shí)間: 2025-3-22 11:37
Non Radially Pulsating Wolf-Rayet Stars initial mass 100 M. losing mass through stellar wind. The periods range from half an hour to a feu hours. The duration of this instability phase is rather short, of the order of a feu e-folding times, uhich are of a feu thousand years.作者: precede 時(shí)間: 2025-3-22 14:53
https://doi.org/10.1007/978-94-009-3901-1Galaxy; Variation; galaxies; star; stars; stellar; turbulence作者: Exuberance 時(shí)間: 2025-3-22 18:35 作者: 小說 時(shí)間: 2025-3-23 01:07 作者: 飲料 時(shí)間: 2025-3-23 03:52
Two Comments on the β Cephei Variable 12 LacertaeAccording to a popular notion, the dominant pulsation mode in the g Cephei variables is radial. There is, however, at least one exception to this rule. The exception is 12 Lacertae.作者: 熱心助人 時(shí)間: 2025-3-23 06:22
978-94-010-8232-7D. Reidel Publishing Company, Dordrecht, Holland 1987作者: 為現(xiàn)場 時(shí)間: 2025-3-23 10:19 作者: Minuet 時(shí)間: 2025-3-23 16:18 作者: MOTTO 時(shí)間: 2025-3-23 21:50 作者: Countermand 時(shí)間: 2025-3-23 23:56
er hinaus noch eine Pers?nlichkeit oder Institution den . erhalten. — Der ., richtet den Wettbewerb im Auftrag des . aus. Am Wettbewerb zum Preis k?nnen ausschlie?lich Produkte und Kommunikationsleistungen teilnehmen, die in den vorangegangenen fünf Jahren bereits eine regionale, nationale oder inte作者: 得意人 時(shí)間: 2025-3-24 04:25 作者: 知識(shí) 時(shí)間: 2025-3-24 06:43 作者: CRUMB 時(shí)間: 2025-3-24 12:46
Yoji Osakier hinaus noch eine Pers?nlichkeit oder Institution den . erhalten. — Der ., richtet den Wettbewerb im Auftrag des . aus. Am Wettbewerb zum Preis k?nnen ausschlie?lich Produkte und Kommunikationsleistungen teilnehmen, die in den vorangegangenen fünf Jahren bereits eine regionale, nationale oder inte作者: seduce 時(shí)間: 2025-3-24 17:31 作者: LIMN 時(shí)間: 2025-3-24 22:45 作者: 樂意 時(shí)間: 2025-3-25 02:20
Jean-Marie Vreuxem Avantgardeprojekt ... war endgültig ein Anbieter für alle geworden“, der ?auch die MTV-und ebay-Generation“ anspricht und bei dem ?das Marketing zunehmend pr?zisere Vorgaben liefert“, konstatiert Bernd Polster in seinem Buch ?Braun. 50 Jahre Produktinnovationen“. Die (historische) Gleichung Diete作者: 整潔 時(shí)間: 2025-3-25 06:50
Henny J. G. L. M. Lamersgn kann darüber hinaus noch eine Pers?nlichkeit oder Institution den . erhalten. ----- Dem . kommt als Preis der Preise eine herausragende Bedeutung für innovative Gestaltungsleistungen in Deutschland zu. Der ., richtet den Wettbewerb im Auftrag des . aus. Am Wettbewerb zum Preis k?nnen ausschlie?li作者: vitrectomy 時(shí)間: 2025-3-25 10:54 作者: 業(yè)余愛好者 時(shí)間: 2025-3-25 15:28 作者: Fretful 時(shí)間: 2025-3-25 18:37 作者: dominant 時(shí)間: 2025-3-25 22:59 作者: muffler 時(shí)間: 2025-3-26 03:57 作者: Truculent 時(shí)間: 2025-3-26 05:39 作者: mucous-membrane 時(shí)間: 2025-3-26 11:05
0067-0057 s held a Chair for Stellar Astrophysics, later changed into Space Physics, since 1958. Cees de Jager, as he prefers to be called by his friends, has had an active and successful life in science. His interest in astronomy was raised by his father under the clear skies of Celebes (Indonesia). He start作者: GRAZE 時(shí)間: 2025-3-26 14:01
Instabilities Due to Convection and Rotations..The instabilities due to rotation are briefly reviewed. Some of them are likely to generate a mild turbulence, whose nature and efficiency are still a matter of conjecture. In early-type stars, this turbulence may mix the radiative envelope to some extent, and it may also deliver mechanical energy to their outer layers.作者: 過于平凡 時(shí)間: 2025-3-26 18:01
Massive Stars in Nearby Galaxiesnance lines have very low outflow velocities compared to galactic stars, and no P Cygni profiles, suggesting that there may be significant differences in mass loss mechanisms among Local Group galaxies, as a consequence of different metal1icities. The UV interstellar extinction in both galaxies appears like the LMC and not like the Galaxy.作者: 流浪 時(shí)間: 2025-3-26 23:43
The Unstable 06.5f?p Star HD 148937 and its Interstellar Environmentlex (semimajor axis ? 1 pc) with HD 148937 located in the apparent center of symmetry. Here we report on observations of these nebulosities (narrow-band CCD imaging, IDS spectrophotometry, high resolution (△V ? 7 km sec.) spectroscopy) in an attempt to establish a consistent model of HD 148937 and its nebulosities.作者: 窒息 時(shí)間: 2025-3-27 04:25 作者: Derogate 時(shí)間: 2025-3-27 09:08
Observations and Interpretations of Stellar Pulsations, RR Lyrae, ? Cephei and δ Scuti stars..For two classes the complex variability of stars is described in detail: the 53 Persei stars and the supergiants. In these two classes non-radial modes have been identified and the complete mode identification has still to be largely improved.作者: photopsia 時(shí)間: 2025-3-27 09:34
Theory of Vibrational Instabilities in Luminous Early Type Stars pulsation amplitudes are limited to relatively small values by nonlinear effects. Although the pulsations may enhance the mass loss from very massive stars, for ZAMS stars radiative driving forces will probably always dominate the mass loss rate.作者: 從屬 時(shí)間: 2025-3-27 16:25 作者: 歌曲 時(shí)間: 2025-3-27 18:22
Stellar Instabilities in the Upper Part of the Hertzsprung-Russell Diagramorkshop and thus contributed to its success. I think the Workshop greatly helped in clarifying ideas on the questions why there are no stars brighter or more massive than certain upper limits, and what happens to stars close to these limits.作者: Rct393 時(shí)間: 2025-3-28 00:08 作者: 擁護(hù)者 時(shí)間: 2025-3-28 02:13 作者: 效果 時(shí)間: 2025-3-28 09:51 作者: 捏造 時(shí)間: 2025-3-28 12:42
Theory of Non-Radial Pulsations in Massive Early-Type Starsstars. Variation in modal-property with stellar evolution is then discussed with the help of the so-called propagation diagram. Problems of vibrational instabilities, effects of rotation, possible consequence of existence of non-axisymmetric waves on the stellar atmosphere are briefly discussed.作者: 全部 時(shí)間: 2025-3-28 15:12 作者: Obituary 時(shí)間: 2025-3-28 19:25 作者: 原諒 時(shí)間: 2025-3-28 23:11 作者: colloquial 時(shí)間: 2025-3-29 06:56 作者: Neuropeptides 時(shí)間: 2025-3-29 09:48
Instabilities Due to Convection and Rotationies. Some of the instabilities which are associated with convection are discussed, with the possible consequences on the behavior of the surface layers..The instabilities due to rotation are briefly reviewed. Some of them are likely to generate a mild turbulence, whose nature and efficiency are stil作者: Feature 時(shí)間: 2025-3-29 13:50 作者: 磨碎 時(shí)間: 2025-3-29 19:08 作者: Gnrh670 時(shí)間: 2025-3-29 22:07 作者: defenses 時(shí)間: 2025-3-30 03:22 作者: 發(fā)芽 時(shí)間: 2025-3-30 06:49 作者: 受傷 時(shí)間: 2025-3-30 11:02 作者: Interregnum 時(shí)間: 2025-3-30 12:41
Non Radially Pulsating Wolf-Rayet Stars initial mass 100 M. losing mass through stellar wind. The periods range from half an hour to a feu hours. The duration of this instability phase is rather short, of the order of a feu e-folding times, uhich are of a feu thousand years.作者: Neolithic 時(shí)間: 2025-3-30 20:37
gern. Gutes Design tr?gt zu Akzeptanz bei den Kunden bei, f?rdert die Produkt-Qualit?t, hilft dem Unternehmer, bessere Preise zu erzielen, transportiert das Image eines Unternehmens und ist ein unverzichtbares Marketing-Instrument. — Der . verleiht den . als Ehrenpreis in Form von Urkunden. Er wird 作者: PHIL 時(shí)間: 2025-3-30 21:14 作者: Amplify 時(shí)間: 2025-3-31 04:55
G. Burkigern. Gutes Design tr?gt zu Akzeptanz bei den Kunden bei, f?rdert die Produkt-Qualit?t, hilft dem Unternehmer, bessere Preise zu erzielen, transportiert das Image eines Unternehmens und ist ein unverzichtbares Marketing-Instrument. — Der . verleiht den . als Ehrenpreis in Form von Urkunden. Er wird 作者: 削減 時(shí)間: 2025-3-31 05:29 作者: 植物群 時(shí)間: 2025-3-31 11:21 作者: aphasia 時(shí)間: 2025-3-31 16:51
Dietrich Baade erz?hlt er, werde er heute noch gelegentlich Mr. Braun genannt. Er sagt es so nebenbei und distanziert, als wolle er diese Anmerkung gleich wieder beiseite schieben. Ein bisschen Stolz, ja Genugtuung klingen da allerdings doch durch. Und warum auch nicht? Zur ganz pers?nlichen wie zur designhistori
