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Titlebook: Reviews in Modern Astronomy; Variabilities in Sta Gerhard Klare Conference proceedings 1992 Springer-Verlag Berlin Heidelberg 1992 Accretio

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书目名称Reviews in Modern Astronomy
副标题Variabilities in Sta
编辑Gerhard Klare
视频video
丛书名称Reviews in Modern Astronomy
图书封面Titlebook: Reviews in Modern Astronomy; Variabilities in Sta Gerhard Klare Conference proceedings 1992 Springer-Verlag Berlin Heidelberg 1992 Accretio
描述The International Scientific Spring Meeting of the Astronomische Ge­ sellschaft (AG) held at Bamberg in April 1991 was devoted to "Vari­ abilities in Stars and Galaxies". Time-dependent phenomena are observed in a wide range of as­ tronomical objects. They are caused by different physical mechanisms (for example by pulsation, by accretion, or by dramatic eruptive events in connection with mass outflow) producing observable intensity vari­ ations through all wavelengths. Many of the papers in this volume are concerned with galactic stars showing such behaviour (for ex­ ample cataclysmic variables, symbiotic stars, luminous blue variables (LBVs) and novae). Intrinsic variations of the, magnetic field struc­ ture on observable time scales are, for instance, a peculiarity of cool, solar-like stars and represent a useful tool to study differential rotation and cycles of activity. Recent results on the investigation of gas motions in the inner regions of the Milky Way system, a study of the bipolar galaxy M 82, observations of variable extragalactic radio sources, the variability of emission lines in active galactic nuclei (AGN) as well as continuum variations of quasars and AGN are disc
出版日期Conference proceedings 1992
关键词Accretion; active galactic nuclei; astronomy; quasar
版次1
doihttps://doi.org/10.1007/978-3-642-77543-7
isbn_softcover978-3-642-77545-1
isbn_ebook978-3-642-77543-7Series ISSN 0941-1445
issn_series 0941-1445
copyrightSpringer-Verlag Berlin Heidelberg 1992
The information of publication is updating

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Accretion Disc Phenomena,e areas is reviewed in depth. Instead I have selected subtopics of current interest. Similarly the references given in each section are not intended to be complete, but should enable the interested reader to get quickly into the literature.
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Luminous Blue Variables; Quiescent and Eruptive States, the LBVs define an inclined instability strip in a range of absolute magnitudes and temperatures of − 8 ≳ M ≳ − 10 and 10 000 ≲ T ≲ 35 000 K, respectively. The most luminous LBVs are the hottest ones. The spectra of LBVs in minimum phase show (dependent on luminosity) characteristics of Ofpe/WN9 tr
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Observational Aspects of Stellar Seismology,ompared to helioseismology which already has a large number of outstanding results to show that could be achieved only seismologically, stellar seismology is still closer to its infancy. On the other hand, asteroseismology bears an even greater promise than its solar counterpart because it is not li
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