Mass Loss from Red Giants

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Publisher : Springer Science & Business Media
ISBN 13 : 940095428X
Total Pages : 316 pages
Book Rating : 4.4/5 (9 download)

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Book Synopsis Mass Loss from Red Giants by : Mark Morris

Download or read book Mass Loss from Red Giants written by Mark Morris and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 316 pages. Available in PDF, EPUB and Kindle. Book excerpt: Red giant and supergiant stars have long been favorites of professional 6 and amateur astronomers. These enormous stars emit up to 10 times more energy than the Sun and, so, are easy to study. Some of them, specifically the pulsating long-period variables, significantly change their size, brightness, and color within about a year, a time scale of interest to a single human being. Some aspects of the study of red giant stars are similar to the study of pre-main-sequence stars. For example, optical astronomy gives us a tantalizing glimpse of star forming regions but to really investi gate young stars and protostars requires infrared and radio astronomy. The same is true of post-main-sequence stars that are losing mass. Optical astronomers can measure the atomic component of winds from red giant stars that are undergoing mass loss at modest rates 6 (M $ 10- M9/yr.). But to see dust grains and molecules properly, 5 especially in stars with truly large mass loss rates, ~ 10- M9/yr, one requires IR and radio astronomy. As this stage of copious mass loss only lasts for ~105 years one might be tempted to ask, "who cares?".

Mass Loss from Red Giants

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Publisher : Springer
ISBN 13 : 9789027720757
Total Pages : 0 pages
Book Rating : 4.7/5 (27 download)

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Book Synopsis Mass Loss from Red Giants by : Mark Morris

Download or read book Mass Loss from Red Giants written by Mark Morris and published by Springer. This book was released on 1985-08-31 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt: Red giant and supergiant stars have long been favorites of professional 6 and amateur astronomers. These enormous stars emit up to 10 times more energy than the Sun and, so, are easy to study. Some of them, specifically the pulsating long-period variables, significantly change their size, brightness, and color within about a year, a time scale of interest to a single human being. Some aspects of the study of red giant stars are similar to the study of pre-main-sequence stars. For example, optical astronomy gives us a tantalizing glimpse of star forming regions but to really investi gate young stars and protostars requires infrared and radio astronomy. The same is true of post-main-sequence stars that are losing mass. Optical astronomers can measure the atomic component of winds from red giant stars that are undergoing mass loss at modest rates 6 (M $ 10- M9/yr.). But to see dust grains and molecules properly, 5 especially in stars with truly large mass loss rates, ~ 10- M9/yr, one requires IR and radio astronomy. As this stage of copious mass loss only lasts for ~105 years one might be tempted to ask, "who cares?".

Mass Loss in Red Giants and Supergiants

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Publisher :
ISBN 13 :
Total Pages : 31 pages
Book Rating : 4.:/5 (287 download)

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Book Synopsis Mass Loss in Red Giants and Supergiants by : Frederick Charles Sanner

Download or read book Mass Loss in Red Giants and Supergiants written by Frederick Charles Sanner and published by . This book was released on 1976 with total page 31 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Astrophysics of Red Supergiants

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Publisher :
ISBN 13 : 9780750313292
Total Pages : 0 pages
Book Rating : 4.3/5 (132 download)

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Book Synopsis Astrophysics of Red Supergiants by : Emily M. Levesque

Download or read book Astrophysics of Red Supergiants written by Emily M. Levesque and published by . This book was released on 2017 with total page 0 pages. Available in PDF, EPUB and Kindle. Book excerpt: "Astrophysics of Red Supergiants' is the first book of its kind devoted to our current knowledge of red supergiant stars, a key evolutionary phase that is critical to our larger understanding of massive stars. It provides a comprehensive overview of the fundamental physical properties of red supergiants, their evolution, and their extragalactic and cosmological applications. It serves as a reference for researchers from a broad range of fields (including stellar astrophysics, supernovae, and high-redshift galaxies) who are interested in red supergiants as extreme stages of stellar evolution, dust producers, supernova progenitors, extragalactic metallicity indicators, members of massive binaries and mergers, or simply as compelling objects in their own right. The book is accessible to a range of experience levels, from graduate students up to senior researchers."--Source : résumé de l'éditeur.

The Influence of Mass Loss on the Evolution of a Red Giant Star of 5 Solar Masses

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Publisher :
ISBN 13 :
Total Pages : 206 pages
Book Rating : 4.:/5 (29 download)

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Book Synopsis The Influence of Mass Loss on the Evolution of a Red Giant Star of 5 Solar Masses by : Jack Eugene Forbes

Download or read book The Influence of Mass Loss on the Evolution of a Red Giant Star of 5 Solar Masses written by Jack Eugene Forbes and published by . This book was released on 1966 with total page 206 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Asymptotic Giant Branch Stars

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Publisher : Springer Science & Business Media
ISBN 13 : 9780387008806
Total Pages : 578 pages
Book Rating : 4.0/5 (88 download)

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Book Synopsis Asymptotic Giant Branch Stars by : Harm J. Habing

Download or read book Asymptotic Giant Branch Stars written by Harm J. Habing and published by Springer Science & Business Media. This book was released on 2004 with total page 578 pages. Available in PDF, EPUB and Kindle. Book excerpt: This book deals with stars during a short episode before they undergo a ma jor, and fatal, transition. Soon the star will stop releasing nudear energy, it will become a planetary nebula for abrief but poetic moment, and then it will turn into a white dwarf and slowly fade out of sight. Just before this dramatic change begins the star has reached the highest luminosity and the largest diameter in its existence, and while it is a star detectable in galaxies beyond the Local Group, its structure contains already the inconspicuous white dwarf it will become. It is called an "asymptotic giant branch star" or "AGB star". Over the last 30 odd years AGB stars have become a topic of their own although individual members of this dass had already been studied for cen turies without realizing what they were. In the early evolution, so called "E-AGB"-phase, the stars are a bit bluer than, but otherwise very similar to, what are now called red giant branch stars (RGB stars). It is only in the sec ond half of their anyhow brief existence that AGB stars differ fundamentally from RGB stars.

The Influence of Mass Loss on the Evolution of a Red Giant of 5 Solar Masses

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Publisher :
ISBN 13 :
Total Pages : 186 pages
Book Rating : 4.:/5 (442 download)

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Book Synopsis The Influence of Mass Loss on the Evolution of a Red Giant of 5 Solar Masses by : Jack Eugene Forbes

Download or read book The Influence of Mass Loss on the Evolution of a Red Giant of 5 Solar Masses written by Jack Eugene Forbes and published by . This book was released on 1966 with total page 186 pages. Available in PDF, EPUB and Kindle. Book excerpt:

Physical Processes in Red Giants

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Publisher : Springer Science & Business Media
ISBN 13 : 9400984928
Total Pages : 483 pages
Book Rating : 4.4/5 (9 download)

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Book Synopsis Physical Processes in Red Giants by : I. Iben

Download or read book Physical Processes in Red Giants written by I. Iben and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 483 pages. Available in PDF, EPUB and Kindle. Book excerpt: In recent years, it has become clear that the red-giant phase is one of the most dramatic periods in a star's life, when all of its parts become involved in ways that have both direct and indirect observational consequences. This is most particularly true of low- and intermediate mass stars during the second ascent of the giant branch. Such stars bring to their surfaces products of nucleosynthesis currently taking place in their deep interiors, they pulsate as Mira variables, develop extended outward-flowing atmospheres that may exhibit maser properties, and shed great quantities of matter, sometimes highly processed, into the inter stellar medium. The manner in which processed matter is brought to the surface is far from being completely explained, and the precise mechanism or mechanisms whereby matter is ejected from the stellar surface (whether by deposition of Alfven waves, radiation pressure on grains, or as a consequence of so me large scale envelope instability) has yet to be elucidated to every one's satisfaction. The purpose of the second workshop in Astrophysics, organized by the "Advanced School of Astronomy", was to bring together experts on all the physical processes occurring in red giants in an effort to emphasize the interrelatedness of these individual processes, and to encourage a dia logue among experts that might serve to initiate a synthesis, or at least sharpen our understanding of the most important problems to address in the future.

Molecular Radio Line Observations of Mass Loss from Red Giants

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Publisher :
ISBN 13 :
Total Pages : pages
Book Rating : 4.:/5 (186 download)

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Book Synopsis Molecular Radio Line Observations of Mass Loss from Red Giants by : Hans Olofsson

Download or read book Molecular Radio Line Observations of Mass Loss from Red Giants written by Hans Olofsson and published by . This book was released on 1988 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt:

Understanding Stellar Evolution

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Publisher : CRC Press
ISBN 13 : 9780750312790
Total Pages : 342 pages
Book Rating : 4.3/5 (127 download)

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Book Synopsis Understanding Stellar Evolution by : Henny J. G. L. M. Lamers

Download or read book Understanding Stellar Evolution written by Henny J. G. L. M. Lamers and published by CRC Press. This book was released on 2018-02-28 with total page 342 pages. Available in PDF, EPUB and Kindle. Book excerpt: 'Understanding Stellar Evolution' is based on a series of graduate-level courses taught at the University of Washington since 2004, and is written for physics and astronomy students and for anyone with a physics background who is interested in stars. It describes the structure and evolution of stars, with emphasis on the basic physical principles and the interplay between the different processes inside stars such as nuclear reactions, energy transport, chemical mixing, pulsation, mass loss, and rotation. Based on these principles, the evolution of low- and high-mass stars is explained from their formation to their death. In addition to homework exercises for each chapter, the text contains a large number of questions that are meant to stimulate the understanding of the physical principles. An extensive set of accompanying lecture slides is available for teachers in both Keynote(R) and PowerPoint(R) formats.

Mass-loss from Giant and Supergiant Stars

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Publisher :
ISBN 13 :
Total Pages : 17 pages
Book Rating : 4.:/5 (249 download)

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Book Synopsis Mass-loss from Giant and Supergiant Stars by : P. G. Wannier

Download or read book Mass-loss from Giant and Supergiant Stars written by P. G. Wannier and published by . This book was released on 1985 with total page 17 pages. Available in PDF, EPUB and Kindle. Book excerpt:

The Galaxies of the Local Group

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Publisher : Cambridge University Press
ISBN 13 : 1139429655
Total Pages : 348 pages
Book Rating : 4.1/5 (394 download)

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Book Synopsis The Galaxies of the Local Group by : Sidney Bergh

Download or read book The Galaxies of the Local Group written by Sidney Bergh and published by Cambridge University Press. This book was released on 2000-05-15 with total page 348 pages. Available in PDF, EPUB and Kindle. Book excerpt: The Local Group is a small cluster of galaxies that includes the Milky Way. At least half of all galaxies in the Universe are thought to belong to similar groups. This authoritative volume provides a comprehensive synthesis of what is known about the Local Group. It begins with a summary of each member galaxy, as well as those galaxies previously regarded as possible members. The book examines the mass, stability and evolution of the Local Group as a whole and includes many important previously unpublished results and conclusions. With clarity, Professor van den Bergh provides a masterful summary of all that is known about the galaxies of the Local Group and their evolution, and expertly places this knowledge in the wider context of on-going studies of galaxy formation and evolution, the cosmic distance scale, and the conditions in the early Universe.

Mass Loss from Stars

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Publisher : Springer Science & Business Media
ISBN 13 : 9401034052
Total Pages : 349 pages
Book Rating : 4.4/5 (1 download)

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Book Synopsis Mass Loss from Stars by : M. Hack

Download or read book Mass Loss from Stars written by M. Hack and published by Springer Science & Business Media. This book was released on 2012-12-06 with total page 349 pages. Available in PDF, EPUB and Kindle. Book excerpt: Proceedings from the Second Trieste Colloquium on Astrophysics, September 12-17, 1968

Science with Astronomical Near-Infrared Sky Surveys

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Publisher : Springer
ISBN 13 :
Total Pages : 312 pages
Book Rating : 4.3/5 (91 download)

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Book Synopsis Science with Astronomical Near-Infrared Sky Surveys by : N. Epchtein

Download or read book Science with Astronomical Near-Infrared Sky Surveys written by N. Epchtein and published by Springer. This book was released on 1994-08-31 with total page 312 pages. Available in PDF, EPUB and Kindle. Book excerpt: Outstanding progress in near-infrared detection technology and in real-time image processing has led astronomers to start undertaking all-sky surveys in the 1--2 mum range (project DENIS in Europe and 2MASS in the U.S.A.), surveys which will have a considerable impact in various areas of astronomy. This book gathers the contributions of more than 80 specialists involved in fields of interest as different as low mass stars, late stages of stellar evolution, star formation, stellar populations of the Galaxy and the Magellanic Clouds, the local structure of the Universe, and observational cosmology. It describes the impact on these fields of the exhaustive data bases and catalogs of stars and galaxies that these surveys will provide. The considerable interest of these documents for the future of infrared space and ground-based projects and the complementarity with other currently ongoing or planned surveys in other spectral ranges are emphasized.

Molecular Radio Line Observation of Mass Loss from Red Giants

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ISBN 13 :
Total Pages : pages
Book Rating : 4.:/5 (946 download)

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Book Synopsis Molecular Radio Line Observation of Mass Loss from Red Giants by :

Download or read book Molecular Radio Line Observation of Mass Loss from Red Giants written by and published by . This book was released on 1988 with total page pages. Available in PDF, EPUB and Kindle. Book excerpt:

New Worlds, New Horizons in Astronomy and Astrophysics

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Publisher : National Academies Press
ISBN 13 : 0309157994
Total Pages : 324 pages
Book Rating : 4.3/5 (91 download)

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Book Synopsis New Worlds, New Horizons in Astronomy and Astrophysics by : National Research Council

Download or read book New Worlds, New Horizons in Astronomy and Astrophysics written by National Research Council and published by National Academies Press. This book was released on 2011-02-04 with total page 324 pages. Available in PDF, EPUB and Kindle. Book excerpt: Driven by discoveries, and enabled by leaps in technology and imagination, our understanding of the universe has changed dramatically during the course of the last few decades. The fields of astronomy and astrophysics are making new connections to physics, chemistry, biology, and computer science. Based on a broad and comprehensive survey of scientific opportunities, infrastructure, and organization in a national and international context, New Worlds, New Horizons in Astronomy and Astrophysics outlines a plan for ground- and space- based astronomy and astrophysics for the decade of the 2010's. Realizing these scientific opportunities is contingent upon maintaining and strengthening the foundations of the research enterprise including technological development, theory, computation and data handling, laboratory experiments, and human resources. New Worlds, New Horizons in Astronomy and Astrophysics proposes enhancing innovative but moderate-cost programs in space and on the ground that will enable the community to respond rapidly and flexibly to new scientific discoveries. The book recommends beginning construction on survey telescopes in space and on the ground to investigate the nature of dark energy, as well as the next generation of large ground-based giant optical telescopes and a new class of space-based gravitational observatory to observe the merging of distant black holes and precisely test theories of gravity. New Worlds, New Horizons in Astronomy and Astrophysics recommends a balanced and executable program that will support research surrounding the most profound questions about the cosmos. The discoveries ahead will facilitate the search for habitable planets, shed light on dark energy and dark matter, and aid our understanding of the history of the universe and how the earliest stars and galaxies formed. The book is a useful resource for agencies supporting the field of astronomy and astrophysics, the Congressional committees with jurisdiction over those agencies, the scientific community, and the public.

Mass Loss from Stars

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ISBN 13 :
Total Pages : 366 pages
Book Rating : 4.3/5 (91 download)

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Book Synopsis Mass Loss from Stars by : Margherita Hack

Download or read book Mass Loss from Stars written by Margherita Hack and published by . This book was released on 1969 with total page 366 pages. Available in PDF, EPUB and Kindle. Book excerpt: