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Titlebook: Mass-Losing Pulsating Stars and their Circumstellar Matter; Observations and The Y. Nakada,M. Honma,M. Seki Book 2003 Springer Science+Busi

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發(fā)表于 2025-3-21 18:14:23 | 只看該作者 |倒序?yàn)g覽 |閱讀模式
書目名稱Mass-Losing Pulsating Stars and their Circumstellar Matter
副標(biāo)題Observations and The
編輯Y. Nakada,M. Honma,M. Seki
視頻videohttp://file.papertrans.cn/626/625307/625307.mp4
叢書名稱Astrophysics and Space Science Library
圖書封面Titlebook: Mass-Losing Pulsating Stars and their Circumstellar Matter; Observations and The Y. Nakada,M. Honma,M. Seki Book 2003 Springer Science+Busi
描述Editing the proceedings of a scientific meeting is not an easy task. Sometimes people who give an excellent talk do not send the manuscript 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 volume. We regret that we cannot put in this volume a few posters that we failed to receive before the editorial work. The workshop was planned as a small meeting with less than fifty attendants because the city of Sendai was far from the most of the active institutions. However, the number of submitted papers exceeded the SOC‘s expectation; many interesting contributions had to be scheduled in the poster session. Still, the oral sessions were so tight that many participants might have felt frustrated for the shortage of discussions. The organizers of the workshop have to apologize to the attendants for the inconvenience caused from such a happy underestimate about the size of the workshop.
出版日期Book 2003
關(guān)鍵詞Astrometry; Bulge; Galaxy; space astrometry; stellar
版次1
doihttps://doi.org/10.1007/978-94-010-0139-7
isbn_softcover978-94-010-3968-0
isbn_ebook978-94-010-0139-7Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightSpringer Science+Business Media Dordrecht 2003
The information of publication is updating

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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
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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 (
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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
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