The Lives And Death Throes Of Massive Stars Iau S329

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The Lives and Death-Throes of Massive Stars (IAU S329)

Author : J.J. Eldridge,John C. Bray,Liam A.S. McClelland,Lin Xiao
Publisher : Cambridge University Press
Page : 500 pages
File Size : 43,5 Mb
Release : 2017-08-31
Category : Science
ISBN : 1107170060

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The Lives and Death-Throes of Massive Stars (IAU S329) by J.J. Eldridge,John C. Bray,Liam A.S. McClelland,Lin Xiao Pdf

Research on massive stars is undergoing a period of rapid progress, with long-held convictions being shown to be incomplete. While these stars are relatively few in number, they are the main driver of chemical and dynamical evolution in galaxies through their stellar winds and explosive deaths in core-collapse supernovae. Furthermore the impact of massive stars is widely recognized in many areas, as they are often used as tools to interpret the conditions and processes arising in different environments. In parallel, the development of new instrumentation, analysis techniques and dedicated surveys across all possible wavelengths have delivered large amounts of exquisite new data. These data are now providing a harsh test for the current state-of-the-art theoretical calculations of massive star birth, evolution and death. IAU Symposium 329 covers these topics and is therefore an invaluable resource for researchers in the field of massive stars and their evolution.

Death of Massive Stars (IAU S279)

Author : Peter W. A. Roming,Nobuyuki Kawai,Elena Pian
Publisher : Cambridge University Press
Page : 478 pages
File Size : 50,6 Mb
Release : 2012-09-20
Category : Science
ISBN : 1107019796

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Death of Massive Stars (IAU S279) by Peter W. A. Roming,Nobuyuki Kawai,Elena Pian Pdf

Massive stars end their lives in fiery explosions and are manifest as core collapse supernovae (CCSNe) or gamma-ray bursts (GRBs). In rare cases, a highly stripped massive star explodes and exhibits properties of both CCSNe and GRBs. In contrast, there are clear cases in which no bright supernova is found to be associated with a GRB, and vice versa. The quest in understanding supernovae and GRBs, and the connection between them, has raised many questions. Since the elements synthesized in the explosion of massive stars are the building blocks for much of the visible Universe, it is important to understand the life cycle of these massive stars. IAU Symposium 279 brings together international leaders who study CCSNe and GRBs to discuss their environments and hosts, progenitors, and subsequent explosions, as well as multiwavelength observations of these objects and their implications as cosmological probes, particularly in the very early Universe.

Massive Stars as Cosmic Engines (IAU S250)

Author : International Astronomical Union. Symposium
Publisher : Cambridge University Press
Page : 616 pages
File Size : 51,6 Mb
Release : 2008-07-17
Category : Science
ISBN : 0521874726

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Massive Stars as Cosmic Engines (IAU S250) by International Astronomical Union. Symposium Pdf

Reviews our current understanding of the life, evolution and death of massive stars; for researchers and graduate students.

The Death of Massive Stars

Author : International Astronomical Union. Symposium
Publisher : Unknown
Page : 455 pages
File Size : 55,9 Mb
Release : 2012
Category : Gamma ray bursts
ISBN : OCLC:812651932

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The Death of Massive Stars by International Astronomical Union. Symposium Pdf

Massive Star Birth (IAU S227)

Author : Riccardo Cesaroni,Marcello Felli,Ed Churchwell,Macolm Walmsley
Publisher : Cambridge University Press
Page : 0 pages
File Size : 55,8 Mb
Release : 2006-01-23
Category : Science
ISBN : 052185198X

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Massive Star Birth (IAU S227) by Riccardo Cesaroni,Marcello Felli,Ed Churchwell,Macolm Walmsley Pdf

Massive stars, those with between 10 and 100 times the mass of the Sun, are among the rarest stars of all. They live fast and die young, but during their short lives produce the most dramatic effects on the surrounding interstellar medium in terms of dynamics, ionization, and chemical enrichment. Until a few decades ago massive star birth was literally shrouded in mystery, since these stars are born deep inside dense clouds of swirling dust and gas that obscure our view. At IAU S227, more than 200 of the world's leading astronomers presented a cornucopia of new results concerning the birth and infancy of massive stars. These proceedings show the achievements reached in this field, due to observations in the radio at mm and sub-mm wavelengths and in the infrared, and to theoretical models that simulate what happens in the cradle of a massive star.

Very Massive Stars in the Local Universe

Author : Jorick S. Vink
Publisher : Springer
Page : 0 pages
File Size : 54,7 Mb
Release : 2014-11-07
Category : Science
ISBN : 3319095951

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Very Massive Stars in the Local Universe by Jorick S. Vink Pdf

This book presents the status of research on very massive stars in the Universe. While it has been claimed that stars with over 100 solar masses existed in the very early Universe, recent studies have also discussed the existence and deaths of stars up to 300 solar masses in the local Universe. This represents a paradigm shift for the stellar upper-mass limit, which may have major implications far beyond the field of stellar physics. The book comprises 7 chapters, which describe this discipline and provide sufficient background and introductory content for graduate (PhD) students and researchers from different branches of astronomy to be able to enter this exciting new field of very massive stars.

New Windows on Massive Stars (IAU S307)

Author : Georges Meynet,Cyril Georgy,José Groh,Philippe Stee
Publisher : Cambridge University Press
Page : 0 pages
File Size : 49,6 Mb
Release : 2015-02-12
Category : Science
ISBN : 110707858X

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New Windows on Massive Stars (IAU S307) by Georges Meynet,Cyril Georgy,José Groh,Philippe Stee Pdf

Massive stars play a crucial role in the Universe: they are important drivers for the photometric and chemical evolution of galaxies; they are sources of important elements, including those necessary for life; and, with their strong winds and supernova explosions, they feed the interstellar medium with momentum and kinetic energy, impacting on the star formation rate. Knowledge of the evolution of massive stars is important not only for stellar physics, but also for probing the evolution of galaxies and their star formation histories throughout cosmic time. This volume provides an introduction to these topics and to the techniques used to investigate the properties of massive stars, including asteroseismology, spectropolarimetry, and interferometry. It highlights synergies between these new techniques and more classical methods, to create a synthetic view of massive stars, leading researchers towards new and innovative solutions to the most topical questions regarding the evolution of massive stars.

Massive Stars Near and Far (IAU S361)

Author : Jonathan Mackey,Jorick S. Vink,Nicole St-Louis
Publisher : Cambridge University Press
Page : 0 pages
File Size : 40,5 Mb
Release : 2024-05-31
Category : Science
ISBN : 1108490654

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Massive Stars Near and Far (IAU S361) by Jonathan Mackey,Jorick S. Vink,Nicole St-Louis Pdf

A Massive Star Odyssey

Author : International Astronomical Union. Symposium
Publisher : Unknown
Page : 840 pages
File Size : 41,7 Mb
Release : 2003
Category : Starbursts
ISBN : UVA:X004717359

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A Massive Star Odyssey by International Astronomical Union. Symposium Pdf

The Origin of Outflows in Evolved Stars (IAU S366)

Author : Leen Decin,Albert Zijlstra,Clio Gielen
Publisher : Cambridge University Press
Page : 0 pages
File Size : 43,5 Mb
Release : 2023-01-19
Category : Science
ISBN : 1108490794

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The Origin of Outflows in Evolved Stars (IAU S366) by Leen Decin,Albert Zijlstra,Clio Gielen Pdf

The prime parameter determining the evolution of a star is its mass. Any modification to the stellar mass has large repercussions on its evolutionary path. Both low-mass and massive stars are known to power strong stellar winds at the end of their lives. These winds determine the type of the stellar end product and the amount by which these stars contribute to the chemical enrichment of the interstellar medium, ultimately providing the building blocks of planets and life. A proper understanding of stellar evolution and the building blocks in the Universe cannot be achieved without a detailed understanding of stellar winds. IAU Symposium 366 provides an overview of state-of-the-art observational and theoretical studies on the origin of winds in low-mass and massive evolved stars, with topics including binarity, enrichment of the interstellar medium, astrochemistry, and theoretical, observational and numerical constraints on stellar outflows.

Birth and Evolution of Massive Stars and Stellar Groups

Author : Wilfried Boland,Hugo Van Woerden
Publisher : Unknown
Page : 377 pages
File Size : 49,7 Mb
Release : 1985
Category : Stars
ISBN : OCLC:1158638785

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Birth and Evolution of Massive Stars and Stellar Groups by Wilfried Boland,Hugo Van Woerden Pdf

The Classical Journal

Author : Anonim
Publisher : Unknown
Page : 428 pages
File Size : 47,9 Mb
Release : 1822
Category : Classical philology
ISBN : HARVARD:AH6HDG

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The Classical Journal by Anonim Pdf

Abstractiones

Author : Richard (Sophista)
Publisher : Auctores Britannici Medii Aevi
Page : 0 pages
File Size : 46,6 Mb
Release : 2016
Category : Philosophy
ISBN : 0197265979

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Abstractiones by Richard (Sophista) Pdf

The Abstractiones is a work in medieval logic from the second half of the 13th century. Clearly a product of the British university culture and much cited, quoted and imitated, it is attributed in two manuscripts to 'Master Richard the Sophist'. This Richard is referred to by other philosophers and logicians as 'The Master of Abstractions' - an honorific title which indicates that his work was a standard textbook. The Abstractiones is a collection of sophismata, or logical puzzles of increasing complexity and difficulty which have been gathered under logical operators like 'all'. Each sophisma is introduced by a proposition that appears to be both provably true and provably false, like 'God knows whatever he knew'. The Master determines the truth or falsity of the proposition and analyses the defects of the arguments that have been offered by detecting logical fallacies, equivocal expressions and the like. The work as we have it is clearly the result of a process of development, modification, and interpolation, probably extending over at least a generation. Although there came to be works that imitated the Abstractions and followed some of its plan and style, these are 'descendants, ' rather than variations. The Abstractions gives us a better sense than does an independent and original work of medieval logic like William of Ockham's Summa Totius Logicae of how instruction in techniques of argumentation and reasoning, often of a fairly sophisticated sort, was carried on in British universities in the latter part of the 13th century and well into the 14th century.