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Titlebook: Mass Outflows from Stars and Galactic Nuclei; Proceedings of the S Luciana Bianchi,Roberto Gilmozzi Conference proceedings 1988 Kluwer Acad

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书目名称Mass Outflows from Stars and Galactic Nuclei
副标题Proceedings of the S
编辑Luciana Bianchi,Roberto Gilmozzi
视频video
丛书名称Astrophysics and Space Science Library
图书封面Titlebook: Mass Outflows from Stars and Galactic Nuclei; Proceedings of the S Luciana Bianchi,Roberto Gilmozzi Conference proceedings 1988 Kluwer Acad
描述The objective of this workshop was to put together observational and theoretical works on outflows from different kinds of astrophysical objects, occurring on different scales and at various evolutionary phases, and to discuss the impact of observations from future space missions. For the stars, we thought to follow throughout the evolution the relevance (rates and dynamical rrodes) of the mass loss phenomenon, e. g. to explain how and when massive stars loose most of their ini tial mass to end up with typical WD masses. The observations of the solar wind were included for being a unique case where the origin and propagation of the outflow can be resolved. We thought that the comparison with similar phenomena occurring in galactic outflows would be fruitful, as demonstrated by recent works on galactic winds and jets. The interest of having this workshop in Torino came because there are groups in this area, at the Astronomical Observatory and at the Institute of Physics of the University, involved in the theoretical and observational studies of outflows from astrophysical objects. The members of the Scientific Organizing Conmi ttee were: V. Castellani, C. Cesarski, P. Conti, A. Ferr
出版日期Conference proceedings 1988
关键词Galaxy; Quasar; magnetosphere; relativistic jet; stars; stellar
版次1
doihttps://doi.org/10.1007/978-94-009-2941-8
isbn_softcover978-94-010-7824-5
isbn_ebook978-94-009-2941-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
issn_series 0067-0057
copyrightKluwer Academic Publishers 1988
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Requirements for Theoretical Models of Outflowsd indisputable evidence for mass loss from the α Her system, the topic of mass loss has grown to be a major research area in astrophysics. The review papers presented at this Workshop summarize the current status of this field.
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Masses of Planetary Nebulae and their Central Starsosity)..The central star mass can only be determined at present from its luminosity and evolutionary considerations. The present status is summarized. A range of masses between 0.5 and 1M are found. Some inconsistancies between theory and observations are discussed.
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Mass Loss and Post-Asymptotic Giant-Branch Evolutionremnant depends very sensitively on the initial condition prevailing during its formation. By this very reason the somewhat approximative calculations of Paczynski (1971) failed to give a satisfactory explanation of the evolution of the central stars (CPN).
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0067-0057 ects, occurring on different scales and at various evolutionary phases, and to discuss the impact of observations from future space missions. For the stars, we thought to follow throughout the evolution the relevance (rates and dynamical rrodes) of the mass loss phenomenon, e. g. to explain how and
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