標(biāo)題: Titlebook: Mass-Losing Pulsating Stars and their Circumstellar Matter; Observations and The Y. Nakada,M. Honma,M. Seki Book 2003 Springer Science+Busi [打印本頁] 作者: 共用 時間: 2025-3-21 18:14
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書目名稱Mass-Losing Pulsating Stars and their Circumstellar Matter讀者反饋學(xué)科排名
作者: 狗舍 時間: 2025-3-21 20:42 作者: agenda 時間: 2025-3-22 03:47
Luminosities of AGB Variabless in the LMC and galactic globular clusters. Hipparcos observations indicate that most Miras in the solar neighbourhood are consistent with such a relation. There are two groups of stars with luminosities that are apparently greater than the PL relation would predict: (1) in the LMC and SMC there ar作者: 火花 時間: 2025-3-22 07:47 作者: COUCH 時間: 2025-3-22 12:08
Stellar Sources in the Isogal Intermediate Bulge Fields In combination with near-infrared (IJK.) data of DENIS survey, we discuss the nature of the ISOGAL sources, their luminosities, the interstellar extinction and the mass-loss rates. A large fraction of the detected sources at 15 . are AGB stars above the RGB tip, a number of them show an excess in (作者: 尖叫 時間: 2025-3-22 15:25 作者: promote 時間: 2025-3-22 18:17 作者: 偏狂癥 時間: 2025-3-22 22:15
Nonlinear Properties of the Semi-Regular Variable Starsulsation mechanism. An application to R Sct thus shows that the irregular lightcurve is the result of the nonlinear interaction of two highly nonadiabatic pulsation modes, namely a linearly unstable, low frequency mode, and the second mode that, although linearly stable, gets entrained through a 2:1作者: 人工制品 時間: 2025-3-23 04:54 作者: LINES 時間: 2025-3-23 05:44 作者: 機(jī)械 時間: 2025-3-23 11:43
The Galactic Kinematics of Mira Variablesewed. Local Miras in the 145-200day period range show a large asymmetric drift and a high net outward motion in the Galaxy. Interpretations of this phenomenon are considered and (following Feast and Whitelock 2000) it is suggested that they are outlying members of the bulge-bar population and indica作者: 愚蠢人 時間: 2025-3-23 14:09 作者: Harass 時間: 2025-3-23 18:45 作者: craving 時間: 2025-3-24 02:09 作者: 發(fā)牢騷 時間: 2025-3-24 03:13 作者: 被詛咒的人 時間: 2025-3-24 06:39
The Extended Atmosphere and Evolution of the RV Tauri Star, R Scutistars, but rather commonly seen in Mira variables. The period evolution of this star does not fit with an ordinary post-AGB scenario. Therefore, we argue an alternative choice of the evolutional stage; R Sct is not a post-AGB star but an AGB star in the helium-burning phase of the thermal-pulse cycl作者: vocation 時間: 2025-3-24 12:36 作者: 愛國者 時間: 2025-3-24 18:46
e claim as supermodel Heidi Klum? Many scholars of chemistry do not hesi- te to point out that the names associated with “name reactions” are often not the actual inventors. For instance, the Arndt-Eistert reaction has nothing to do with either Arndt or Eistert, Pummerer did not discover the “Pummer作者: 指耕作 時間: 2025-3-24 22:49
P. R. Wood latest references to these name reactions.Gives representatI don‘t have my name on anything that I don‘t really do. –Heidi Klum Can the organic chemists associated with so-called “Named Reactions” make the same claim as supermodel Heidi Klum? Many scholars of chemistry do not hesi- te to point out 作者: 存在主義 時間: 2025-3-24 23:44 作者: Inexorable 時間: 2025-3-25 04:05 作者: URN 時間: 2025-3-25 10:57 作者: 似少年 時間: 2025-3-25 15:19
D. K. Ojha,A. Omont,ISOGAL Teame claim as supermodel Heidi Klum? Many scholars of chemistry do not hesi- te to point out that the names associated with “name reactions” are often not the actual inventors. For instance, the Arndt-Eistert reaction has nothing to do with either Arndt or Eistert, Pummerer did not discover the “Pummer作者: alcohol-abuse 時間: 2025-3-25 19:49
Arūnas Ku?inskas,Lennart Lindegren,Toshihiko Tanabé,Vladas Vansevi?iuse Kr?fte zu. In der Literatur sind Namen h?ufig kreativer Ausdruck der Figurenschicksale: Da sie zwischen Wirklichkeit und Imagination angesiedelt sind, bleiben sie oft hintergründig und geheimnisvoll – das verlangt nach fantasievollen, überzeugenden Deutungen.Angesichts der Relevanz literarischer N作者: adipose-tissue 時間: 2025-3-25 21:37 作者: 啜泣 時間: 2025-3-26 00:28
e Kr?fte zu. In der Literatur sind Namen h?ufig kreativer Ausdruck der Figurenschicksale: Da sie zwischen Wirklichkeit und Imagination angesiedelt sind, bleiben sie oft hintergründig und geheimnisvoll – das verlangt nach fantasievollen, überzeugenden Deutungen.Angesichts der Relevanz literarischer N作者: 倫理學(xué) 時間: 2025-3-26 07:04 作者: Hectic 時間: 2025-3-26 12:32 作者: 枕墊 時間: 2025-3-26 15:56 作者: Bureaucracy 時間: 2025-3-26 19:24
se, and/or are the first to popularize the transformation. Regardless of the controversial history underlying certain named reactions, it is the students of organic chemistry who benefit the most from the - taloging of reactions by name. Indeed, it is with education in mind that Dr. Jack Li has mast作者: N斯巴達(dá)人 時間: 2025-3-26 21:37
Sachiyo Noda,Mine Takeutise, and/or are the first to popularize the transformation. Regardless of the controversial history underlying certain named reactions, it is the students of organic chemistry who benefit the most from the - taloging of reactions by name. Indeed, it is with education in mind that Dr. Jack Li has mast作者: GRILL 時間: 2025-3-27 03:20
D. K. Ojha,A. Omont,ISOGAL Teamse, and/or are the first to popularize the transformation. Regardless of the controversial history underlying certain named reactions, it is the students of organic chemistry who benefit the most from the - taloging of reactions by name. Indeed, it is with education in mind that Dr. Jack Li has mast作者: preeclampsia 時間: 2025-3-27 07:09 作者: 會犯錯誤 時間: 2025-3-27 09:39 作者: barium-study 時間: 2025-3-27 15:42 作者: 剝削 時間: 2025-3-27 19:33
Masayuki Y. Fujimoto,Takuma Sudaas Wunderkind, Tristan und Der Tod in Venedig von Thomas Mann. Der Band schlie?t mit Betrachtungen zur Figur des Ogers in M?rchen und Texten unter anderem von Oskar Loerke und Michel Tournier.978-3-7329-8997-3Series ISSN 1868-8306 Series E-ISSN 2940-8520 作者: Carminative 時間: 2025-3-28 00:33 作者: 獨(dú)特性 時間: 2025-3-28 05:02 作者: Leisureliness 時間: 2025-3-28 08:22
P. R. Wood history underlying certain named reactions, it is the students of organic chemistry who benefit the most from the - taloging of reactions by name. Indeed, it is with education in mind that Dr. Jack Li has mast978-3-540-30031-1作者: 割讓 時間: 2025-3-28 10:50
Maria-Rosa L. Cioni history underlying certain named reactions, it is the students of organic chemistry who benefit the most from the - taloging of reactions by name. Indeed, it is with education in mind that Dr. Jack Li has mast978-3-540-30031-1作者: ANTIC 時間: 2025-3-28 17:07 作者: 潛移默化 時間: 2025-3-28 21:23 作者: inferno 時間: 2025-3-29 02:19 作者: ARIA 時間: 2025-3-29 04:25
Three Aspects of Red Giant Studies in the Magellanic Cloudsity function carries informations about the star formation rate in the Clouds and it can be mathematically related to their history. Most AGB stars vary their magnitude in a few to several hundred years time; the one epoch DENIS magnitudes for both Large and Small Magellanic Cloud AGB stars outline the same relations as a function of period作者: CORE 時間: 2025-3-29 10:35
Structure and Evolution of AGB Stars: Current Understandings and Beyondto the formation and early evolution of our galaxy by these studies. Finally, we discuss the importance of non-standard effects in understanding the actual evolution of AGB stars and introduce some recent attempts to reveal their roles in the internal mixing and nucleosynthesis作者: Obverse 時間: 2025-3-29 12:15
Mass-Losing and Pulsating AGB Stars in the Magellanic Cloudsavailable model grid, and (3) the period-mass loss rate relation for C-rich SMC stars seems to follow that derived for Galactic carbon-rich Miras, suggesting no explicit dependence of mass loss rate on metallicity作者: affinity 時間: 2025-3-29 18:16 作者: 種族被根除 時間: 2025-3-29 23:00 作者: Myosin 時間: 2025-3-30 01:28 作者: Irrepressible 時間: 2025-3-30 04:54
Photometric Properties of Long-Period Variables in the Large Magellanic Cloudtigated. Stars with large amplitudes and high periodicities were distributed on the only one strip amongst multiple structure on the LMC period-luminosity relation. In the CMD, the five strips were located in the order of the period. The stars with characterized light curves were also discussed作者: 人造 時間: 2025-3-30 09:14
Stellar Sources in the Isogal Intermediate Bulge Fieldsnction and the mass-loss rates. A large fraction of the detected sources at 15 . are AGB stars above the RGB tip, a number of them show an excess in ([7]-[15])o and (K.-[15])o colors, characteristic of mass-loss. The latter, especially (K.-[15])o, allow estimation of the mass-loss rates (.) and show their distribution in the range 10. to 10. M./yr作者: 故意釣到白楊 時間: 2025-3-30 14:36
GAIA: AGB Stars as Tracers of Star Formation Histories in the Galaxy and Beyondt numbers of AGB stars in the Galaxy and beyond. Reliable ages of AGB stars can be determined to distances of ~200 kpc in a wide range of ages and metallicities, allowing star formation histories to be studied in a diversity of astrophysical environments作者: 下船 時間: 2025-3-30 17:46 作者: kyphoplasty 時間: 2025-3-30 21:02
Regular and Irregular Pulsations of Luminous Blue Variablesing through the stellar atmosphere. Ballistic motions of the outermost layers on the dynamic time scale of the atmosphere are interrupted by strong compressional shock waves. The deposition of energy and momentum leads to atmospheric stratifications that differ significantly from what prevails if hydrostatic stratification is assumed作者: Endearing 時間: 2025-3-31 00:55
Period Evolution in Mira Variablesongest period Miras. In the case of R Hya, the period change was accompanied by a dramatic change in mass-loss rate, consistent with the mass-loss formalism of Vassiliadis & Wood. Their formalism then predicts that the mass-loss rates of the longest period Miras (. > 400days) may fluctuate by a factor of 2-3 over time scales of a century作者: 黃油沒有 時間: 2025-3-31 06:12 作者: Ceramic 時間: 2025-3-31 11:41
Time Dependent Modelling of Mass Loss on the AGB .*) that should enable to determine when this instability takes place. Also, I present first results of calculations that follow the outflow on a timescale longer than that of the mass loss modulation (which is typically of the order of a hundred years). This enables to study the effect of stellar evolution on the wind作者: 陶醉 時間: 2025-3-31 15:22
Asymmetric Mass-Loss on the AGB: Examples from IRAS Datas of bi- or quadru-polar shape and will, due to their huge dimensions, probably have started to form already in the AGB phase. If so, then the mass-loss in the AGB phase is not spherically symmetric in a number of cases作者: pacifist 時間: 2025-3-31 18:50
0067-0057 by the deadline. However, this time, thanks to the punctuality of all the participants, we have this excellent volume for the workshop on mass- losing pulsating stars and their circumstellar matter prepared in time. Almost all of the oral presentations including the summary are collected in this vol作者: Adjourn 時間: 2025-3-31 22:06 作者: 大炮 時間: 2025-4-1 05:09
978-94-010-3968-0Springer Science+Business Media Dordrecht 2003作者: 進(jìn)取心 時間: 2025-4-1 08:17 作者: Outmoded 時間: 2025-4-1 13:50
Characteristics of AGB Stars in the Isogal, Macho and Other DatabasesThis contribution summarizes briefly some previous findings based on ISOGAL, MACHO and DENIS observations and goes on to include outlines of two projects now in progress:作者: impaction 時間: 2025-4-1 18:07
