標題: Titlebook: Stellar Pulsations; Impact of New Instru J.C. Suárez,R. Garrido,J. Christensen-Dalsgaard Book 2013 Springer-Verlag Berlin Heidelberg 2013 A [打印本頁] 作者: HABIT 時間: 2025-3-21 19:59
書目名稱Stellar Pulsations影響因子(影響力)
書目名稱Stellar Pulsations影響因子(影響力)學(xué)科排名
書目名稱Stellar Pulsations網(wǎng)絡(luò)公開度
書目名稱Stellar Pulsations網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Stellar Pulsations被引頻次
書目名稱Stellar Pulsations被引頻次學(xué)科排名
書目名稱Stellar Pulsations年度引用
書目名稱Stellar Pulsations年度引用學(xué)科排名
書目名稱Stellar Pulsations讀者反饋
書目名稱Stellar Pulsations讀者反饋學(xué)科排名
作者: 金哥占卜者 時間: 2025-3-21 20:57
The Spectroscopic Observations of CoRoT Asteroseismic Targets with HARPSPS spectrograph attached to the 3.6m-ESO telescope in the framework of two consecutive Large Programmes. We discuss its use to study line-profile variations and we report on a specific result obtained for the δ Sct star HD 170699.作者: 大包裹 時間: 2025-3-22 03:07 作者: Acumen 時間: 2025-3-22 07:56
First Detection of Period Doubling in a BL Herculis Type Star: Observations and Theoretical Modelsoskalik (ApJ 391:736, 1992). The star, with .. = 2. 4 d, is located in the Galactic bulge and was discovered with OGLE-III photometry. We present new nonlinear convective models, which, together with recent evolutionary tracks, put constraints on the stellar parameters. In particular, we estimate the mass and metallicity of the object.作者: Ornament 時間: 2025-3-22 10:10
Astrophysics and Space Science Proceedingshttp://image.papertrans.cn/s/image/877163.jpg作者: 非實體 時間: 2025-3-22 14:18 作者: 表示向下 時間: 2025-3-22 19:03
978-3-642-44326-8Springer-Verlag Berlin Heidelberg 2013作者: DRAFT 時間: 2025-3-22 21:22
Stellar Pulsations978-3-642-29630-7Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: annexation 時間: 2025-3-23 03:01 作者: 疼死我了 時間: 2025-3-23 06:22 作者: 密碼 時間: 2025-3-23 09:42
verfahren für die Spurenanalyse von Elementen, Elementspezies und organischen Verbindungen im Mikrogramm/L- und Nanogramm/L-Bereich. Als Empfehlung für den Praktiker und als Anleitung für eigene Methodenentwicklungen werden 30 erprobte Applikationen beschrieben.978-3-642-62548-0978-3-642-56492-5作者: CLASP 時間: 2025-3-23 14:11
ctly the same as those of the solution with nonzero surface tension under numerical noise. The solution of the Saffman-Taylor problem without surface tension is similar to the solution for the equation of cellular flames in the case of the combustion of gas mixtures.作者: 讓你明白 時間: 2025-3-23 21:33
Takafumi Sonoi,Hiromoto Shibahashiire’s towns — Corby and Wellingborough — in 1980/1. The success of the JLB scheme in those areas was such that the procedures and practices developed there were implemented countywide by the mid-1980s.作者: 弄臟 時間: 2025-3-24 01:37
Natallia Sudnik,Alexander Kholtyginire’s towns — Corby and Wellingborough — in 1980/1. The success of the JLB scheme in those areas was such that the procedures and practices developed there were implemented countywide by the mid-1980s.作者: JEER 時間: 2025-3-24 05:47
C. C. Lovekin,J. A. Guzikrother regions.. . This work will be of interest to students and researchers in criminology and criminal justice, particularly with an interest in police studies and corruption, as well as related fields such a978-3-030-00412-5978-3-030-00413-2Series ISSN 2192-8533 Series E-ISSN 2192-8541 作者: 瑪瑙 時間: 2025-3-24 09:08 作者: 最初 時間: 2025-3-24 12:56
Eva Mundprecht,Herbert J. Muthsam coupled with a clear focus on ethical issues, provide a lucid picture of the future of police training in both educational and law enforcement contexts. In addition, the book‘s training templates are not only 978-1-4899-8762-4978-1-4614-0745-4作者: inscribe 時間: 2025-3-24 18:06 作者: interpose 時間: 2025-3-24 23:05 作者: sebaceous-gland 時間: 2025-3-25 03:01 作者: G-spot 時間: 2025-3-25 03:59
Achim Weisshaben. Bei der Analyse einiger Erz?hlf?den — dargestellt in den Kapiteln 6.3, 6.4 und 6.7 — zeigte sich überdies ein weiterer prinzipieller Unterschied zwischen zwei Gruppierungen innerhalb des Typus .: zwischen solchen, für die Polen . der letzte Wert ist, und solchen, für die dies nur . zutrifft.作者: POINT 時間: 2025-3-25 09:12 作者: Popcorn 時間: 2025-3-25 11:47
Ennio Poretti,Monica Rainer,Luciano Mantegazza,Michele Floquet,Philippe Mathias,Pedro Amado,Conny Aend policy development, and leadership concepts. These emerging paradigms and technologies, coupled with a clear focus on ethical issues, provide a lucid picture of the future of police training in both educational and law enforcement contexts. In addition, the book‘s training templates are not only 作者: reflection 時間: 2025-3-25 15:56 作者: Magnificent 時間: 2025-3-25 20:46
Hiromoto Shibahashi,Hiroyuki Ishimatsund policy development, and leadership concepts. These emerging paradigms and technologies, coupled with a clear focus on ethical issues, provide a lucid picture of the future of police training in both educational and law enforcement contexts. In addition, the book‘s training templates are not only 作者: mastoid-bone 時間: 2025-3-26 01:37
Mickael Pasek,Bertrand Georgeot,Fran?ois Lignières,Daniel R. Reesend policy development, and leadership concepts. These emerging paradigms and technologies, coupled with a clear focus on ethical issues, provide a lucid picture of the future of police training in both educational and law enforcement contexts. In addition, the book‘s training templates are not only 作者: 儀式 時間: 2025-3-26 06:21
Fernando Pena,Robert Deupree,Wilfried Beslinnd policy development, and leadership concepts. These emerging paradigms and technologies, coupled with a clear focus on ethical issues, provide a lucid picture of the future of police training in both educational and law enforcement contexts. In addition, the book‘s training templates are not only 作者: filicide 時間: 2025-3-26 11:23
nd policy development, and leadership concepts. These emerging paradigms and technologies, coupled with a clear focus on ethical issues, provide a lucid picture of the future of police training in both educational and law enforcement contexts. In addition, the book‘s training templates are not only 作者: Oscillate 時間: 2025-3-26 14:19
R. Szabó,Z. Kolláth,L. Molnár,K. Kolenberg,D. W. Kurtz,WG#13 membersnd policy development, and leadership concepts. These emerging paradigms and technologies, coupled with a clear focus on ethical issues, provide a lucid picture of the future of police training in both educational and law enforcement contexts. In addition, the book‘s training templates are not only 作者: 生存環(huán)境 時間: 2025-3-26 18:57
R. Smolec,I. Soszyński,P. Moskalik,A. Udalski,M. K. Szymański,M. Kubiak,G. Pietrzyński,?. Wyrzykowsknd policy development, and leadership concepts. These emerging paradigms and technologies, coupled with a clear focus on ethical issues, provide a lucid picture of the future of police training in both educational and law enforcement contexts. In addition, the book‘s training templates are not only 作者: 信條 時間: 2025-3-26 21:58
1570-6591 s also discussed. These Proceedings are distinguished by?the format of the conference, which brings together a variety of related but different topics not found in other meetings of this nature..978-3-642-44326-8978-3-642-29630-7Series ISSN 1570-6591 Series E-ISSN 1570-6605 作者: biosphere 時間: 2025-3-27 02:42
Book 2013lsations (Granada, September 2011). These results are leading to a re-appraisal of our views on stellar pulsation in some stars and posing some new and unexpected challenges. The very important and exciting role played by innovative ground-based observational techniques, such as interferometric meas作者: Hemoptysis 時間: 2025-3-27 06:07
Vibrational Instability of Metal-Poor Low-Mass Main-Sequence Starsthose of Pop I stars, the stars showing γ Dor-type pulsation are substantially less massive than in the case of Pop I stars. We demonstrate that those modes are unstable for about 1 .. stars in the metal-poor case.作者: 咽下 時間: 2025-3-27 09:28
Non-radial Pulsation and Magnetic Fields of OB Stars the large-scale structures in the stellar wind. Results of searching for the polarimetric line profile variability (pLPV) in the spectra of OB stars are also reported. We find that the pattern of LPV can differ for the left and right polarized components of stellar radiation.作者: 晚間 時間: 2025-3-27 16:31
Some Thoughts About the Blazhko Effect for RR Lyrae Variable Pulsationsmaterial opacity an its dependence on temperature and density. Current linear theory for pulsation calculations using my much improved pulsation code show that two beating modes (one radial and another nonradial) may exist for an explanation of those few pulsating RR Lyrae, amplitude varying variable stars.作者: 輕觸 時間: 2025-3-27 18:57 作者: Minutes 時間: 2025-3-28 00:41
Stellar Pulsations and Stellar Evolution: Conflict, Cohabitation, or Symbiosis?s of stellar physics are pointed out as well, for which it is hoped that seismology—or in general the analysis of stellar pulsations—will help to resolve them. The limits of this symbiosis will be discussed as well.作者: Bronchial-Tubes 時間: 2025-3-28 04:56 作者: 冥界三河 時間: 2025-3-28 07:51
Traditional Approximation for Low-Frequency Modes in Rotating Stars and A Working Hypothesis About Ere, we point out that very low frequency oscillations become leaky waves. A working hypothesis is then proposed to explain mass loss in Be stars as episodic wave leakage associated with gradual angular-momentum transport due to prograde modes.作者: FRET 時間: 2025-3-28 11:53
Modelling Stellar Convection and Pulsation in Multidimensions Using the ANTARES Codesfer. We then present the basic parameters of the Cepheid we study more closely. For that star we provide a short discussion of patterns of the . and the . convection zones and the interaction with pulsation seen in the . work or atmospheric structures.作者: Stable-Angina 時間: 2025-3-28 14:54
Periodicities Within the Frequency Spectra of δ Scuti Stars Observed by ,～ 50% of the sub-sample shows a clear pattern. Moreover, we found three objects with almost the same KIC physical parameters showing the same value of the pattern. We suggest that the pattern is a sign of a large-separation-like structure.作者: escalate 時間: 2025-3-28 20:16 作者: 多嘴 時間: 2025-3-29 00:31 作者: 一小塊 時間: 2025-3-29 03:40 作者: 等級的上升 時間: 2025-3-29 10:47 作者: 和平主義 時間: 2025-3-29 11:26
1570-6591 l ground-based experiments.Edited by international leaders i.Analyses of photometric time series obtained from the .MOST., .CoRoT. and .Kepler. space missions were presented?at the 20th conference on Stellar Pulsations (Granada, September 2011). These results are leading to a re-appraisal of our vie作者: glowing 時間: 2025-3-29 15:37
Stellar Pulsations and Stellar Evolution: Conflict, Cohabitation, or Symbiosis?us history. In many cases results from both methods do not agree. In this review some classical and current cases of disagreement are presented. In some cases these conflicts led to an improvement of the theory of stellar evolution, while in others they still remain unsolved. Some well-known problem作者: 自傳 時間: 2025-3-29 22:41 作者: hypnogram 時間: 2025-3-30 00:59 作者: mosque 時間: 2025-3-30 04:32 作者: 我要威脅 時間: 2025-3-30 09:48 作者: critic 時間: 2025-3-30 13:39
The Spectroscopic Observations of CoRoT Asteroseismic Targets with HARPSPS spectrograph attached to the 3.6m-ESO telescope in the framework of two consecutive Large Programmes. We discuss its use to study line-profile variations and we report on a specific result obtained for the δ Sct star HD 170699.作者: hauteur 時間: 2025-3-30 17:24
Recent Progress and Open Questions in Rapidly Rotating Star Seismologyta together with the advances in modelling the effects of rotation bring fresh perspectives towards a successful comparison between theory and observation. In this short review, the recent progress obtained with 2D oscillation codes is summarized and some open issues are pointed out.作者: creatine-kinase 時間: 2025-3-30 23:54
Traditional Approximation for Low-Frequency Modes in Rotating Stars and A Working Hypothesis About Ece of eigenfunction is expressed in terms of the Hough functions, and the radial dependence is expressed in a form similar to the case of non-rotating stars with only the replacement of the spherical degree with the eigenvalue of the Hough function. Paying attention to the non-zero surface temperatu作者: 刺穿 時間: 2025-3-31 01:12 作者: Ambiguous 時間: 2025-3-31 07:16
Regular Modes in Rapidly Rotating Stars asymptotic method for pressure modes predicts regular frequency spacings in the spectrum of rapidly rotating stars. We give a semi-analytical formula for these spacings that is in good agreement with numerically computed high-frequency modes. This should help to extract from observed spectra import
