標題: Titlebook: Variable and Non-spherical Stellar Winds in Luminous Hot Stars; Proceedings of the I Bernhard Wolf,Otmar Stahl,Alex W. Fullerton Conference [打印本頁] 作者: 無緣無故 時間: 2025-3-21 17:15
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars影響因子(影響力)
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars影響因子(影響力)學科排名
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars網絡公開度
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars網絡公開度學科排名
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars被引頻次
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars被引頻次學科排名
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars年度引用
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars年度引用學科排名
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars讀者反饋
書目名稱Variable and Non-spherical Stellar Winds in Luminous Hot Stars讀者反饋學科排名
作者: 無法破譯 時間: 2025-3-21 23:55 作者: Abrade 時間: 2025-3-22 03:22 作者: LIMIT 時間: 2025-3-22 07:47
Stanislav ?teflcorals. It is designed to serve as a unique reference for upcoming marine researchers and chemists, advanced undergraduate and postgraduate students as well as those interested in marine pollution with respect to heavy metals. The book explains the basics as well as the state-of-the-art regarding he作者: 進步 時間: 2025-3-22 09:54 作者: Ejaculate 時間: 2025-3-22 16:31 作者: Conspiracy 時間: 2025-3-22 19:44 作者: antecedence 時間: 2025-3-23 00:57 作者: grenade 時間: 2025-3-23 05:12
Norman R. Trams,C. I. van Tuyll,Robert H. M. Voors,Alex de Koter,Laurens B. F. M. Waters,Patrick W. tigated. It will be confirmed that 2. bb is due to the alignment of a h. -proton pair. The oscillating behaviour of the 2. bb can explain the variation of the second anomaly in the N=90 isotones. Strong variations of the 2. bb with the neutron number can be explained by the change of the deformation作者: 彩色 時間: 2025-3-23 06:02 作者: 殺子女者 時間: 2025-3-23 10:24 作者: 不透明 時間: 2025-3-23 15:04 作者: 吸氣 時間: 2025-3-23 19:43
Ph. Stee,D. Bonneau,D. Mourard,F. Vakiliilig voneinander unabh?ngig zu machen. Dies ist besonders erwünscht, wenn unterbrochen f?rdernde Anlagen mit Stetigf?rderern zusammenarbeiten. H?ufig werden auch Hochbbunker angewendet, um die F?rderanlagen nicht st?ndig betreiben zu müssen und einen gewissen Vorrat zur Verfügung zu halten, so da? d作者: 笨重 時間: 2025-3-23 23:55
Jon E. Bjorkman die Güter zeitlich und mengenm??ig nach einem genau festgelegten Plan bef?rdert, wobei zweckm??ig alle F?rdervorg?nge von der Aufgabe bis zur Abgabe des Materials weitgehend mechanisiert sein sollten und m?glichst wenig Aufwand für Steuerung, Bedienung und Hilfsarbeiten erfordern. Der F?rderer darf作者: 強所 時間: 2025-3-24 06:24 作者: DENT 時間: 2025-3-24 08:21 作者: 同位素 時間: 2025-3-24 13:45
Inverse spectropolarimetric modelling of hot star wind structure and variability,作者: 健壯 時間: 2025-3-24 16:08 作者: 無價值 時間: 2025-3-24 19:31 作者: Lucubrate 時間: 2025-3-25 00:16
ts (Ernst and Joosse-van Damme 1983, 1989). Environmental pollution was and is independent of political regimes, and unfortunately, in many cases, even independent of the technological conditions of a country, as the metal pollution around metal smelters has demonstrated in former West Germany (Erns作者: menopause 時間: 2025-3-25 07:22 作者: Antigen 時間: 2025-3-25 10:48
Stanislav ?teflpollutants such as heavy metals, (ii) to identify sources of heavy metals in the marine environment,(iii) to inform about route of exposure and uptake of the heavy metal pollutants by corals, (iv) to elaborate about the effect of heavy metal pollutants on the coral reef ecosystems, (v) to discuss th作者: Conflict 時間: 2025-3-25 14:32
Thomas Riviniustotoxic, so the concern about these metals is mainly directed at effects on crop yields and soil productivity. Together with cadmium, zinc may be considered as a mobile and bioavailable metal which may accumulate in crops and human diets (Kiekens, 1995). Food plants which tolerate relatively high co作者: 壓碎 時間: 2025-3-25 18:34
Franz-Josef Zickgrafxcellent means of assisting recognition. As a commonly authigenic in sediments. Positive identi- number of mineral grains have similar optical proper- fication of authigenic minerals is important to avoid ties and morphology, it is equally important to confusion and to help recognition of diagenetic describe 978-94-010-5019-7978-94-011-2308-2作者: COM 時間: 2025-3-25 23:15
Cláudia V. Rodrigues,Ant?nio Mário Magalh?es 500°C, which for lean operating engines is rarely reached under normal engine operation..Due to the high temperature stability of methane, a novel approach has been taken to develop a catalyst system which is able to oxidise methane at low temperatures, via the use of alternative oxidising agents. 作者: Lipoprotein 時間: 2025-3-26 01:02
Antonella Notan defined limits. Critical events like mega knock at high BMEP (engine damage) and autoignition during fault ride though events (grid code non-compliance) must be avoided..The selected strategy involves the measurement of the hydrogen content in natural gas and the pre-definition of various engine o作者: lactic 時間: 2025-3-26 06:39
Norman R. Trams,C. I. van Tuyll,Robert H. M. Voors,Alex de Koter,Laurens B. F. M. Waters,Patrick W. spin spectra in the even mass Hg-isotopes by coupling two quasi-particles to an interacting boson core. This calculation can reproduce the anomalous behaviour of the yrast states around angular momentum 8, 10 and 12. The agreement for the yrast state is similar in an earlier calculation where two q作者: 把手 時間: 2025-3-26 12:14 作者: A保存的 時間: 2025-3-26 16:02
Thomas Eversberg,Anthony F. J. Moffat,Michael Debruyne,John B. Rice,Nikolai Piskunov,Pierre Bastien,under, kr?ftiger Eltern, deren vorzeitige Entbindung auf einen Unglücksfall der Mutter oder einen operativen Eingriff zurückgeht, zu gr??eren Hoffnungen als eine gleichaltrige, gleich gro?e Frühgeburt, die durch eine keimsch?digende Erkrankung der Mutter verursacht ist.作者: 魅力 時間: 2025-3-26 17:39
John C. Brown,Richard Ignace,M. Pianaeb gest?rt, m?gen auch die einzelnen mechanischen F?rdereinrichtungen für sich durchaus einwandfrei arbeiten. Es kann daher nicht genug auf die wichtige Bedingung hingewiesen werden, da? die Neigung der Ladeschurren und schr?gen Beh?lterb?den sorgf?ltig dem F?rdergut angepa?t werden mu?. Dabei ist z作者: fibula 時間: 2025-3-27 00:43
Ph. Stee,D. Bonneau,D. Mourard,F. Vakiliest?rt, m?gen auch die einzelnen mechanischen F?rdereinrichtungen für sich durchaus einwandfrei arbeiten. Es kann daher nicht genug auf die wichtige Bedingung hingewiesen werden, da? die Neigung der Ladeschurren und schr?gen Beh?lterb?den sorgf?ltig dem F?rdergut angepa?t werden mu?. Dabei ist zwisc作者: Disk199 時間: 2025-3-27 01:51 作者: 四指套 時間: 2025-3-27 06:06
Using spectropolarimetry to determine envelope geometry and test variability models for hot star ciFurthermore, spectropolarimetric variability, which is significant in a large fraction of the hot stars observed, provides information about changes occuring in the circumstellar envelope. For example, polarimetric changes provide a critical test of the one-armed density wave models proposed to explain observed V/R variations.作者: ANTH 時間: 2025-3-27 12:53 作者: ARBOR 時間: 2025-3-27 16:58
Rotationally modulated winds of O stars,hree case studies are used to illustrate the patterns of variability that are attributed to rotational modulation and to highlight some open issues connected with this hypothesis. The problems associated with establishing the occurrence of rotational modulation rigorously are also discussed.作者: DEFER 時間: 2025-3-27 19:17 作者: 佛刊 時間: 2025-3-28 00:57
Non-isotropic outflows in the infrared: ISO imaging of LBVs,ed. The structure and intensity distribution of the nebular emission is dependent on the wavelength, indicating a separation between the ionised matter and the dust in the nebulae. Some model calculations are presented for the G79.29+0.46 nebula.作者: heterodox 時間: 2025-3-28 02:46
0075-8450 ere is abundant evidence that essentially all luminous hot-star winds contain time-dependent and anisotropic structures. IAU Colloquium 169 was convened to review the observations of variability and asphericity, to discuss the physical processes that might cause such behavior and to look for evoluti作者: 盤旋 時間: 2025-3-28 06:46 作者: BOLT 時間: 2025-3-28 10:46 作者: 厭煩 時間: 2025-3-28 15:37
Observing hot stars in all four stokes parameters,aneous manner. We briefly outline the technical design of the polarimeter unit and the linear algebraic Mueller calculus for obtaining polarization parameters of any point source. In addition, practical limitations of the optical elements are discussed. We present first results obtained with our spectropolarimeter for three prototype hot-star.作者: Project 時間: 2025-3-28 19:10 作者: Throttle 時間: 2025-3-28 23:07 作者: Exonerate 時間: 2025-3-29 04:32
Rotationally modulated winds of O stars,of the underlying star. This rotational modulation is usually attributed to large scale, persistent structures in the wind, which are thought to be generated and maintained by photospheric processes that alter the emergence of the wind from different regions of the stellar surface. In this review, t作者: Accede 時間: 2025-3-29 07:38 作者: 簡略 時間: 2025-3-29 14:25
Disks of classical be stars,of line profiles in the optical and near-IR region were used in the 70th and 80th, the present progress is done also thanks to interferometric and polarimetric observations. These techniques enable to determine the geometrical parameters of the circumstellar disks directly for the first time. They a作者: 修正案 時間: 2025-3-29 16:20
Short and medium term variability of emission lines in selected southern Be stars, stars, . Cen, was found to be in the process of continued gradual recovery of the Hydrogen emitting disk which had been lost from 1977–1989. During the monitoring period numerous line emission outbursts were observed. A generalized pattern of an outburst cycle is derived from observations of differ作者: notice 時間: 2025-3-29 23:41 作者: faculty 時間: 2025-3-30 01:29
Polarimetric evidence of non-spherical winds,vidences for non-spherically symmetric structures around Luminous Hot Stars from polarimetry and what we can learn with this technique. Polarimetry has added a new dimension to the study of the envelopes of Luminous Blue Variables, Wolf-Rayet stars and B[e] stars, all of which are discussed in some 作者: 軍械庫 時間: 2025-3-30 04:44
Wolf-rayet wind models: Photometric and polarimetric variability,ve localized, enhanced density regions (blobs). Our model is based on a Monte Carlo code that treats all Stokes parameters of the radiation bundle. This study indicates that the blobs must have sizes comparable to the stellar dimension and be near the base of the envelope. These blobs can be interpr作者: magnanimity 時間: 2025-3-30 08:20
Anisotropic outflows from LBVs and Ofpe/WN9 stars,tudy of the outflows around evolved massive stars. It has been established (Nota & Clampin 1997) that most LBVs and Ofpe/WN9 stars are surrounded by associated circumstellar nebulae which have been ejected in some previous phase of their evolution. These nebulae are the fossil record of the interact作者: CHARM 時間: 2025-3-30 15:53 作者: 悄悄移動 時間: 2025-3-30 17:27
Optical interferometry of non-spherical winds,s paper we review some few, yet unique results obtained on P Cyg and Be stars from OLBI observations. We also examine the prospects for studying hot stars winds offered by optical synthesis arrays presently under construction.作者: indignant 時間: 2025-3-30 21:08 作者: 沉思的魚 時間: 2025-3-31 01:01 作者: d-limonene 時間: 2025-3-31 07:31
Physics of radiatively driven winds by high angular resolution observations (HARO), Hα line profile and continuum energy distribution or polarization data). Nevertheless, little has been done to include High Angular Resolution Observations (HARO) in simulations in spite of the fact that such data can strongly constrain radiative wind models. In the following, we shall review recen作者: ciliary-body 時間: 2025-3-31 10:41
Wind-compressed disks,s the recently discovered non-radial force components that may inhibit the formation of the disk and present preliminary investigations of the ionization distribution and associated line profiles in the WCD model.作者: 解決 時間: 2025-3-31 13:42 作者: 陶瓷 時間: 2025-3-31 19:56 作者: Arrhythmia 時間: 2025-3-31 23:42
Short and medium term variability of emission lines in selected southern Be stars,inct differences between different groups of spectral lines. Based on this empirical phenomenology, a schematic picture of the associated ejection of matter into a near-stellar orbit is sketched and similarities between . Cen and other stars will be outlined.作者: tackle 時間: 2025-4-1 05:26 作者: 冰雹 時間: 2025-4-1 09:48
Radio evidence for non-isotropic outflows from hot stars,Radio diagnostics for outflows from hot stars are reviewed and three well-studied examples (WR 140, η Car and MWC 349) are discussed in some detail. The three systems are very different and their radio properties are diverse, but in each case, the radio data provide strong evidence for the presence of equatorially-enhanced outflows.作者: Lucubrate 時間: 2025-4-1 12:50
HST WFPCII observations of the inner HR car nebula,We present Hα observations of the inner region of the HR Carinae nebula. The inner nebula looks clumpy and material appears to be present only to the east of the central star. A jet-like filament stretches away from the central star to the southeast.作者: 課程 時間: 2025-4-1 16:07
Bernhard Wolf,Otmar Stahl,Alex W. FullertonThe IAU-Colloquia are extremely carefully referred and they are used a standard reference for many years.Includes supplementary material: 作者: Transfusion 時間: 2025-4-1 21:56
978-3-662-14210-3Springer-Verlag Berlin Heidelberg 1999作者: RODE 時間: 2025-4-2 00:10
Variable and Non-spherical Stellar Winds in Luminous Hot Stars978-3-540-49062-3Series ISSN 0075-8450 Series E-ISSN 1616-6361
