Effects Of Mass Loss On Stellar Evolution
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Effects Of Mass Loss On Stellar Evolution
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Author : C. Chiosi
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06
Effects Of Mass Loss On Stellar Evolution written by C. Chiosi and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.
The IAU Colloquium No. 59, "The effects of mass loss on Stellar Evolution" was held on September 15-19, 1980 at the International Centre for Theoretical Physics, Miramare, Trieste (Italy), under the auspices of the IAU Executive Co~ mittee and the Italian National Council of Research. The planning of this conference began two years ago du ring the IAU Symposium No. 83 "Mass loss and evolution of 0 type stars" (Qualicum Beach, Victoria, Canada) when we felt that mass loss and its effects on the evolution of stars was too broad a subject for being confined to 0 type stars only. Therefore we thought that a conference dealing with the general problem of mass loss across the whole HR diagram would have been of interest to all people working in the field. The main idea was that bringing together Astronomers and Astrophysicists of the widest range of interests and e~ pertize - all in some way related to the problem of mass loss from stars - would have spurred thorough discussions on the many aspects and implications of this topic. We hope this goal has been achieved. Furthermore, the most recent observational and theoreti cal developments on the problem of mass loss from early ty pe stars avoided this meeting to be a simple updating of the Qualicum Beach Symposium as far as this issue is concerned.
Effects Of Mass Loss On Stellar Evolution
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Author :
language : en
Publisher:
Release Date : 1981
Effects Of Mass Loss On Stellar Evolution written by and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1981 with categories.
Effects Of Mass Loss On Stellar Evolution
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Author :
language : en
Publisher:
Release Date : 1980
Effects Of Mass Loss On Stellar Evolution written by and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1980 with categories.
Effects Of Mass Loss On The Late Stages Of Stellar Evolution
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Author : Sun Kwok
language : en
Publisher:
Release Date : 1987
Effects Of Mass Loss On The Late Stages Of Stellar Evolution written by Sun Kwok and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1987 with Mass loss (Astrophysics) categories.
Mass Loss From Stars And The Evolution Of Stellar Clusters
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Author : Alex de Koter
language : en
Publisher:
Release Date : 2008
Mass Loss From Stars And The Evolution Of Stellar Clusters written by Alex de Koter and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 2008 with Mass loss (Astrophysics) categories.
"In the spring of 2006 a four day international workshop was held in Lunteren, The Netherlands, in honor of the formal retirement of Prof. Henny Lamers. These proceedings provide a comprehensive overview of mass loss in massive stars and of the dynamical fate of clusters. The dynamical evolution of clusters is affected by stellar winds, mass loss outbursts and supernova explosions as well as by the loss of stars in dynamical interactions, thus linking the two central themes of the workshop. It is becoming clear that mass loss by radiation pressure on spectral lines is not only at work in normal O, B, and A stars but also in Luminous Blue Variables and Wolf-Rayet stars. The importance of these line-driven winds relative to outbursts in the Luminous Blue Variable phase of evolution is under debate. A central issue in this discussion is the importance of small and possibly large scale structure in stellar winds and its implications for the measured mass loss rates. These proceedings report on progress establishing wind properties, on theoretical predictions of mass loss and wind structure as a function of stellar properties, and on the effects of mass loss on the evolution of massive stars. As a result of dynamical interactions, clusters may dissolve completely over time. Observational studies of cluster dissolution timescales as a function of cluster formation history and cluster and environmental properties, are at the focus of cluster studies in the last decade. A key topic discussed in this book is whether the old globular clusters we observe today were once similar to present-day massive young clusters. The mass function of the two types of clusters is observed to be different. Is this a result of dynamical evoltuion or were the mass functions different at formation? The 12 invited reviews, 18 contributed talks, 48 poster papers, and two discussion sessions combine to provide and in-depth assessment of both observational and theoretical issues. The book is suitable for researchers and graduate students interested in stellar astrophysics and cluster dynamics."--Provided by publisher.
Effects Of Mass Loss On Stellar Evolution Iau Colloquium No 59 Mirame Trieste Italy 15 19 September 1980
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Author : Cesare Chiosi
language : en
Publisher:
Release Date : 1981
Effects Of Mass Loss On Stellar Evolution Iau Colloquium No 59 Mirame Trieste Italy 15 19 September 1980 written by Cesare Chiosi and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1981 with categories.
Stellar Structure And Evolution
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Author : Rudolf Kippenhahn
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-10-31
Stellar Structure And Evolution written by Rudolf Kippenhahn and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-10-31 with Science categories.
This long-awaited second edition of the classical textbook on Stellar Structure and Evolution by Kippenhahn and Weigert is a thoroughly revised version of the original text. Taking into account modern observational constraints as well as additional physical effects such as mass loss and diffusion, Achim Weiss and Rudolf Kippenhahn have succeeded in bringing the book up to the state-of-the-art with respect to both the presentation of stellar physics and the presentation and interpretation of current sophisticated stellar models. The well-received and proven pedagogical approach of the first edition has been retained. The book provides a comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The models developed to explain the stability, dynamics and evolution of the stars are presented and great care is taken to detail the various stages in a star’s life. Just as the first edition, which remained a standard work for more than 20 years after its first publication, the second edition will be of lasting value not only for students but also for active researchers in astronomy and astrophysics.
Mass Loss And Evolution Of O Type Stars
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Author : P.S. Conti
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06
Mass Loss And Evolution Of O Type Stars written by P.S. Conti and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.
The organization of this Symposium had its beginnings at the International Astronomical Union General Assembly in Grenoble in 1976. The initial "rounding up" of the Scienti fic Organizing Committee was begun by Drs. Snow and Swings; most of us who became the eventual organizing committee met a few times during the Assembly and formulated the essential outlines of the meeting. Extensive correspondence with all the committee subsequently established the program. The idea was to bring together both observers and theoreticians to discuss the stellar winds and mass loss rates and their effects on evolutions of O-type stars. On the observational side, there are now spectroscopic data from the far UV to the near IR regions concerning the stellar winds. There is also information about the free-free emission in the wind from the IR and radio portions of the spectrum. Fortunately, these different detection methods give more or less the same mass loss rate for the one star, s Pup" which has been observed at all wavelengths. One of the intents of the first three sessions of this Symposium is to outline the eXisting data on mass loss rates as it per tains to the O-type stars.
Mass Loss On The Agb And Its Consequences For Stellar Evolution
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Author : Astrophysikalisches Institut Potsdam
language : en
Publisher:
Release Date : 1994
Mass Loss On The Agb And Its Consequences For Stellar Evolution written by Astrophysikalisches Institut Potsdam and has been published by this book supported file pdf, txt, epub, kindle and other format this book has been release on 1994 with categories.
Angular Momentum And Mass Loss For Hot Stars
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Author : L.A. Willson
language : en
Publisher: Springer Science & Business Media
Release Date : 2012-12-06
Angular Momentum And Mass Loss For Hot Stars written by L.A. Willson and has been published by Springer Science & Business Media this book supported file pdf, txt, epub, kindle and other format this book has been release on 2012-12-06 with Science categories.
Fundamental unsolved problems of stellar astrophysics include the effects of angular momentum on stellar structure and evolution, the nature and efficiency of the processes by which angular momentum is redistributed within and lost from stars, and the role that stellar rotation plays in enhancing or driving stellar mass loss. There appears to be a qualitative change in the nature and efficiency of these mechanisms near spectral type FO: hotter (more massive) stars typically retain more angular momentum at least until they reach the main sequence, while cooler stars typically spin down quickly. For the hotter stars, recent work suggests a strong link between the type of pulsation behavior, the mass loss rates, and the rotation velocity. If the same mechanisms are able to drive mass loss from the main sequence A stars, as has recently been proposed, then the current interpretations of a number of observations will be drastically affected: e. g. the ages of clusters may be incorrect by up to a factor of two, and the surface abundances of isotopes of He, Li and Be may no longer give constraints on cosmological nucleosynthesis. There are also effects on the evolution of the abundances of elements in the interstellar medium and on the general evolution of populations of stars. Thus the questions of the mechanisms of angular momentum and mass loss of stars more massive than the sun is important not only for stellar studies but for the foundations of much of modern astrophysics.