標(biāo)題: Titlebook: Variable Stars as Essential Astrophysical Tools; Proceeding of the NA Cafer ?bano?lu Conference proceedings 20001st edition Kluwer Academic [打印本頁] 作者: 初生 時(shí)間: 2025-3-21 19:52
書目名稱Variable Stars as Essential Astrophysical Tools影響因子(影響力)
書目名稱Variable Stars as Essential Astrophysical Tools影響因子(影響力)學(xué)科排名
書目名稱Variable Stars as Essential Astrophysical Tools網(wǎng)絡(luò)公開度
書目名稱Variable Stars as Essential Astrophysical Tools網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Variable Stars as Essential Astrophysical Tools被引頻次
書目名稱Variable Stars as Essential Astrophysical Tools被引頻次學(xué)科排名
書目名稱Variable Stars as Essential Astrophysical Tools年度引用
書目名稱Variable Stars as Essential Astrophysical Tools年度引用學(xué)科排名
書目名稱Variable Stars as Essential Astrophysical Tools讀者反饋
書目名稱Variable Stars as Essential Astrophysical Tools讀者反饋學(xué)科排名
作者: PLE 時(shí)間: 2025-3-21 21:20
Evidence for, and Development of, the Oblique Pulsator ModelThe oblique pulsator model is introduced for the roAp stars in the case of the best-studied star, HR 3831. A detailed discussion of some techniques and pitfalls of frequency analysis is given. Developments of the oblique pulsator model from both theoretical and observational viewpoints are given and problems discussed.作者: 效果 時(shí)間: 2025-3-22 03:26 作者: Immortal 時(shí)間: 2025-3-22 05:32
Asteroseismology of CepheidsThe importance of Cepheids is well known in many fields of astronomy. In this contribution I would like to show how it is possible to obtain indications about the internal structure of a Cepheid and how we can test models of this class of variable stars.作者: Obituary 時(shí)間: 2025-3-22 11:18
978-0-7923-6084-1Kluwer Academic Publishers 2000作者: cartilage 時(shí)間: 2025-3-22 14:51
Variable Stars as Essential Astrophysical Tools978-94-011-4299-1Series ISSN 1389-2185 作者: 忍受 時(shí)間: 2025-3-22 17:49 作者: 誘使 時(shí)間: 2025-3-23 01:12 作者: 套索 時(shí)間: 2025-3-23 02:20
Asteroseismology with A Spatial Resolutionsimilar to helioseismology, the inverse techniques for investigation of a star’s inner structure. Numerous sets of detected and (.) — identifiednormal nonradial modes is crucial for the application of these techniques to stars.作者: 序曲 時(shí)間: 2025-3-23 05:43
Nato Science Series C:http://image.papertrans.cn/v/image/980514.jpg作者: 發(fā)酵劑 時(shí)間: 2025-3-23 11:30
https://doi.org/10.1007/978-94-011-4299-1Astrometry; Fitting; Hipparcos catalog; asteroseismology; astronomy; helioseismology; stellar作者: 騙子 時(shí)間: 2025-3-23 15:36
J?rgen Christensen-Dalsgaard,Woiciech A. Dziembowski作者: 不開心 時(shí)間: 2025-3-23 22:06
J?rgen Christensen-Dalsgaard,Werner D?ppen,Woiciech A. Dziembowski,Joyce A. Guzikdlung des Problems erst m?glich werden lassen. Die Konstruktion von theoretischen Modellen ist typisch für die Physik. Ein . kann man in gewisser Weise mit einer . vergleichen, die das für die aktuelle Fragestellung Wesentliche betont und allen . wegl?sst. Ein Modell ist deshalb stets nur für einen 作者: 剛開始 時(shí)間: 2025-3-23 23:08 作者: Fortify 時(shí)間: 2025-3-24 02:43 作者: 起皺紋 時(shí)間: 2025-3-24 09:36
A. P. Hatzes,D. E. Mkrtichian,A. Kanaanlute Grenzgeschwindigkeit erkl?ren und von der ?quivalenz von Energie und Masse zeugen. Die Lorentz-Transformation bezieht sich nur auf geradlinig gleichf?rmig gegeneinander bewegte Systeme, sagt aber nichts aus über relativ zueinander beschleunigte Systeme.作者: Alcove 時(shí)間: 2025-3-24 11:59 作者: Misgiving 時(shí)間: 2025-3-24 15:24
Ennio Porettilen in mehrere unabh?ngige, gew?hnliche Differentialgleichungen zu zerlegen. Man nennt dieses Verfahren ., das wir im übrigen schon an vielen Stellen dieses . angewendet haben. Natürlich lassen sich nicht alle Probleme .. Es gelingt allerdings insbesondere bei Teilchenbewegungen in einem ..作者: companion 時(shí)間: 2025-3-24 22:42 作者: affluent 時(shí)間: 2025-3-24 23:35
Evolution and Hydrodynamics of Rotating Starser ratio of blue to red supergiants, the region between the end of core hydrogen burning and the beginning of core helium burning in massive stars, and the location of blue loops for some intermediate mass stars).作者: vocation 時(shí)間: 2025-3-25 07:25 作者: entice 時(shí)間: 2025-3-25 11:06
J?rgen Christensen-Dalsgaard,Werner D?ppen,Woiciech A. Dziembowski,Joyce A. Guzikalische Problem galt dabei jeweils als gel?st, sobald die Bahnkurve . eines jeden Massenpunktes aus vorgegebenen Kraftgleichungen abgeleitet war. Bei einem makroskopischen Festk?rper mit seinen etwa . Teilchen pro cm. wird das Konzept des Massenpunktes natürlich fragwürdig. Es ist allerdings auch zu作者: Presbyopia 時(shí)間: 2025-3-25 15:15 作者: Concerto 時(shí)間: 2025-3-25 16:34 作者: Mindfulness 時(shí)間: 2025-3-25 20:26
A. P. Hatzes,D. E. Mkrtichian,A. Kanaanit bzw. von der Invarianz physikalischer Aussagen vom Bezugssystem des Beobachters. Insbesondere handelt die Spezielle Relativit?tstheorie von der Gleichberechtigung aller Inertialsysteme, wobei die überg?nge zwischen den verschiedenen Inertialsystemen allerdings nicht durch Galilei-, sondern durch 作者: DAMP 時(shí)間: 2025-3-26 01:26
D. E. Mkrtichian,A. P. Hatzes,V. E. Panchuknzuführen. Das wird uns in der Statistischen Mechanik wesentlich glatter gelingen. In der Thermodynamik bleibt es gewisserma?en bei einem gefühlsm??igen Selbstverst?ndnis dieses Begriffs..Der Erste Hauptsatz, den wir in diesem Abschnitt formulieren wollen, macht eine Aussage über das Wesen der W?rme作者: 修改 時(shí)間: 2025-3-26 06:10 作者: 遠(yuǎn)地點(diǎn) 時(shí)間: 2025-3-26 11:52
Solar Models and Helioseismologyls with various initial heavy element abundance (.) are also obtained to deduce which . is appropriate. Relative sound speed difference between the Sun and model with diffusion of H and heavy elements and with . = 0.02 is not larger than 0.2%.作者: MITE 時(shí)間: 2025-3-26 13:01 作者: Innocence 時(shí)間: 2025-3-26 17:37 作者: FANG 時(shí)間: 2025-3-26 21:23
Introduction to Asteroseismology of , Scuti Starsere I will discuss what we can learn about the Sun by studying . Scuti stars, as well as what we can learn about stars more massive or evolved than the Sun. I will discuss some of the difficulties in theoretical approaches to asteroseismology for 8 Scuti stars, using FG Virginis, . Scuti, and CD –24° 7599 (also known as XX Pyxidis) as examples.作者: GORGE 時(shí)間: 2025-3-27 01:35 作者: inflame 時(shí)間: 2025-3-27 06:40
Techniques of Collection, Reduction and Analysis of Data of Pulsating Stars IIospheres and coronas. A detailed description is then given on how to correct photometric data for atmospheric extinction. Through a description of a “blind” statistical approach to cluster surveys we will then underline how important information about pulsating variables resides in the class more than in the individual.作者: doxazosin 時(shí)間: 2025-3-27 13:09 作者: Endoscope 時(shí)間: 2025-3-27 15:05 作者: frugal 時(shí)間: 2025-3-27 20:54 作者: 分解 時(shí)間: 2025-3-27 21:56 作者: FEMUR 時(shí)間: 2025-3-28 03:28
Astrophysical Equation of State and Opacitymooth, consistent, valid over a large range of temperatures and densities, and must incorporate the most important astrophysically relevant chemical elements. The equation of state appears as a necessary part of stellar modeling as well as of any opacity calculation. For the latter, it has to provid作者: 整理 時(shí)間: 2025-3-28 08:28 作者: exophthalmos 時(shí)間: 2025-3-28 11:55
The Pulsational Behaviour of Variable Stars in the Lower Part of the Instability Striphe past years a great effort was made by the stellar group of Brera Observatory (E. Antonello, M. Bossi, L. Mantegazza, E. Poretti, F.M. Zerbi) to collect a large amount of photometric and spectroscopic data on . Sct stars, the more numerous class. Observations were carried out using the telescopes 作者: 道學(xué)氣 時(shí)間: 2025-3-28 14:57 作者: Intrepid 時(shí)間: 2025-3-28 21:20 作者: Finasteride 時(shí)間: 2025-3-29 02:07
Techniques of Collection, Reduction and Analysis of Data of Pulsating Stars IIameters through empirical and semi-empirical calibrations as well as how to obtain additional information from the observation in other bands of chromospheres and coronas. A detailed description is then given on how to correct photometric data for atmospheric extinction. Through a description of a “作者: BUDGE 時(shí)間: 2025-3-29 06:28 作者: Femine 時(shí)間: 2025-3-29 08:47
An Introduction to Ap Stars, roAp Stars and the Asteroseismology of roAp Starsous sub-classes. The diffusion hypothesis is explained. A description of how diffusion accounts semi-quantitatively for the CP stars is given. Problems with,the diffusion hypothesis are discussed as are applications of diffusion to other fields of stellar astrophysics. Observations of magnetic field作者: LIKEN 時(shí)間: 2025-3-29 15:14
Multi-Color Observations and Atmospheric Level Effects in roAp Starsis short compared to the geometrical depth at optical depth τ = 1. A derivation showing that we can probe the pulsation over a significant portion of its vertical wavelength is shown. New observations and theoretical advances for Ap star models are then shown supporting this discovery. A comparison 作者: LEVY 時(shí)間: 2025-3-29 16:19 作者: EWE 時(shí)間: 2025-3-29 23:03
Pulsational Radial Velocity Studies of Roap Starsous abundances of elements that are distributed inhomogeneously on the stellar surface. (Some elements are concentrated near the magnetic poles and others are concentrated near the magnetic equator.) The rapidly oscillating Ap stars (roAp) are a pulsating subclass of these objects that oscillate in 作者: Bernstein-test 時(shí)間: 2025-3-30 02:43
Asteroseismology with A Spatial Resolutionsimilar to helioseismology, the inverse techniques for investigation of a star’s inner structure. Numerous sets of detected and (.) — identifiednormal nonradial modes is crucial for the application of these techniques to stars.作者: 水土 時(shí)間: 2025-3-30 07:43 作者: ABIDE 時(shí)間: 2025-3-30 08:52
The Pulsational Behaviour of Variable Stars in the Lower Part of the Instability Striplocated in Merate (0.50 m and 1.02 m; a third telescope having a diameter of 1.32 m will be available in the near future) and in La Silla (European Southern Observatory, Chile; we used the 0.50 m, 0.90 m, 1.0 m to make the photometric observations, the 1.4-m CAT for the spectroscopic ones).作者: 粗魯性質(zhì) 時(shí)間: 2025-3-30 12:29
An Introduction to Ap Stars, roAp Stars and the Asteroseismology of roAp Starss in upper main sequence stars are discussed and the oblique rotator model introduced and explained. Mean light variations from spots on CP stars are shown. The rapidly oscillating Ap stars are introduced, and asteroseismology of these stars is shown in detail for a few stars.作者: Exuberance 時(shí)間: 2025-3-30 17:46 作者: DEFER 時(shí)間: 2025-3-30 21:17
Conference proceedings 20001st editionons of recentlydiscovered Ap stars. This textbook covers almost all kinds of variablestars of widely different characteristics. It will serve as areference text for a very long time to come, not only for specialistsbut also for undergraduate students of physics and astronomy.作者: ROOF 時(shí)間: 2025-3-31 03:32
1389-2185 ty variations of recentlydiscovered Ap stars. This textbook covers almost all kinds of variablestars of widely different characteristics. It will serve as areference text for a very long time to come, not only for specialistsbut also for undergraduate students of physics and astronomy.978-0-7923-6084-1978-94-011-4299-1Series ISSN 1389-2185 作者: 單色 時(shí)間: 2025-3-31 05:47 作者: 強(qiáng)制性 時(shí)間: 2025-3-31 09:30
From Immanuel Kant to Johann Gottlieb Fichte – Concept of Education and German Idealismgs. Every individual being is basically only an imperfect image of possible humanity. Despite the empirical imperfection, every human being has at least potentially the possibility to perfect oneself.作者: Ventilator 時(shí)間: 2025-3-31 13:44 作者: 抗生素 時(shí)間: 2025-3-31 18:26 作者: Jejune 時(shí)間: 2025-3-31 22:45
Werner A. Müller,Stephan Frings,Frank M?hrlend effaced the memory of Kolin; the Convention of Klosterzeven had been disavowed as disgracefully as it was made; Ferdinand of Brunswick was thrusting westwards across the rivers, so that Frederick the Great, hardly sensible as yet of the impending shock of Russian manpower, had room to breathe agai作者: 心胸狹窄 時(shí)間: 2025-4-1 02:52
Fazit,ons wenden sie an. Trotz der vielen Erfolge gibt und gab es immer wieder Vorurteile gegenüber statistisch gewonnenen Einsichten. Sie werden haupts?chlich durch die Unbestimmtheit ihrer Ergebnisse, also durch die in ihnen steckende unangenehme ?Zuf?lligkeit“ gen?hrt.作者: DEI 時(shí)間: 2025-4-1 06:44
Some Smaller Polyoxoanions. Their Synthesis and Characterization in Solution作者: Adjourn 時(shí)間: 2025-4-1 14:04
Acute Renal Failure1°C), shaking chills, and hemoglobinuria. She was treated with Benadryl and Solu-medrol. EKG revealed new Q waves in the inferior leads. Clindamycin, gentamicin, and nafcillin were also administered at this time. Over the next 10 days, urine output decreased, and the serum creatinine concentration i作者: LATHE 時(shí)間: 2025-4-1 16:17
Television Violence and the Youngbis ins 11. Jh. gehalten haben (id., p. 20), obwohl schon in der Mitte des 6. Jh. Slawen in den menschenleeren Gebieten Schlesiens “massiv” auftauchten (id., p. 21). Wenn auch .. und .. den vandalischen Einschlag untersch?tzen, so war doch bis zum Einsetzen der deutschen Kolonisation Oberschlesien g?nzlich slawisiert.作者: Cabinet 時(shí)間: 2025-4-1 22:02
Quantitative Myokardszintigraphie bei KoronaroperationenDarstellung eines me
