Explaining Lithium Enriched Red Giant Branch Stars

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Explaining Lithium Enriched Red Giant Branch Stars

Author : Claudia Aguilera-Gómez
Publisher : Springer
Page : 131 pages
File Size : 47,9 Mb
Release : 2018-11-28
Category : Science
ISBN : 9783030025830

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Explaining Lithium Enriched Red Giant Branch Stars by Claudia Aguilera-Gómez Pdf

This thesis provides new insights into the seemingly anomalous ubiquity of lithium-rich red giant stars. The theory of stellar evolution, one of the most successful models of modern astrophysics, predicts that red giant stars should display negligible levels of lithium (Li) on their surfaces. However, Li-rich giants, defined as those showing more than three times the Li content of the Sun, are found everywhere astronomers look in apparent defiance of established theory. The author addresses this problem, analyzing the different possible explanations for such an anomaly, which include interaction with a binary companion, the production of Li in the interior of the star with its subsequent transport to stellar exteriors, and the stellar interaction with planets. The author focuses on this last possibility, where the Li enrichment may be due to the ingestion of planets or brown dwarfs as the stars in question grew in size while becoming giants. She shows that this process is indeed able to explain an important fraction of giants with Li levels above the three times solar threshold, but that some other mechanism is needed to explain the remaining fraction. While this is an important discovery in its own right, the result that makes this thesis groundbreaking is its demonstration that the threshold between Li-normal and Li-rich is mass dependent rather than a fixed proportion of the Sun’s content. This corrects a fundamental misapprehension of the phenomenon and opens up a new framework in which to understand and solve the problem. Finally, the author presents interesting observational applications and samples with which to test this new approach to the problem of Li enrichment in giants.

Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites

Author : S. Randich,L. Pasquini
Publisher : Springer Science & Business Media
Page : 391 pages
File Size : 45,6 Mb
Release : 2006-09-25
Category : Science
ISBN : 9783540341369

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Chemical Abundances and Mixing in Stars in the Milky Way and its Satellites by S. Randich,L. Pasquini Pdf

This proceedings covers topics from chemical abundances in the different components of the Milky Way and in local group galaxies, via observational and theoretical papers on mixing in stars to big bang nucleosynthesis and galaxy formation and evolution. Like all volumes in the series ESO Astrophysics Symposia, this one gives a comprehensive overview of the forefront of research in this subject. It is a valuable reference for both students and researchers.

Astronomical Applications of Astrometry

Author : M. A. C. Perryman
Publisher : Cambridge University Press
Page : 695 pages
File Size : 43,6 Mb
Release : 2009
Category : Nature
ISBN : 9780521514897

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Astronomical Applications of Astrometry by M. A. C. Perryman Pdf

An authoritative account of the contributions to science made by the Hipparcos satellite, for astronomers, astrophysicists and cosmologists.

Asymptotic Giant Branch Stars

Author : Harm J. Habing,Hans Olofsson
Publisher : Springer Science & Business Media
Page : 578 pages
File Size : 44,5 Mb
Release : 2004
Category : Science
ISBN : 0387008802

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Asymptotic Giant Branch Stars by Harm J. Habing,Hans Olofsson Pdf

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.

Origins of Life

Author : Vlado Valkovic
Publisher : CRC Press
Page : 447 pages
File Size : 43,7 Mb
Release : 2021-11-09
Category : Science
ISBN : 9781000470802

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Origins of Life by Vlado Valkovic Pdf

The primary purpose of this book is to prepare the ground for coordinated efforts aiming to answer the question: where and when life originated. The appearance of life involves three successive stages: i) the formation of chemical elements and their combination to simple molecules, which is the concern of physicists; ii) the evolution of organized complexity in biomolecules and their reactions, which falls within the field of chemistry; iii) the onset of Darwinian evolution after the appearance of the first cell-like structure, which is studied by biologists. This book focuses on the first two steps of this process with chapters exploring topics such as chemical element abundances; galaxies, galactic magnetic fields and cosmic rays; galactic chemical evolution. Key Features: Contains extensive lists of reference and additional reading. Includes new hypotheses concerning the origin of life. Combines consideration from nuclear physics, astrophysics, astro- and geochemistry. Despite its interdisciplinary nature, this book remains accessible to nonexperts, and would be a valuable companion for both experts and laypeople.

Chemical Abundances in the Universe

Author : International Astronomical Union. Symposium
Publisher : Cambridge University Press
Page : 518 pages
File Size : 47,5 Mb
Release : 2010
Category : Cosmic abundances
ISBN : 0521764955

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Chemical Abundances in the Universe by International Astronomical Union. Symposium Pdf

Session I : Primordial nucleosynthesis and the first stars in the Universe -- Session II : First stars in the Galaxy -- Session III : Chemical abundances in the high red-shift Universe -- Session IV : Chemical abundance constraints on mass assembly and star formation in local galaxies and the Milky Way -- Session V : Extrasolar planets: the chemical abundance connection -- Session VI : Abundance surveys and projects in the era of future large telescopes.

Civil Services Chronicle September 2020

Author : Mr. NN OJha
Publisher : CHRONICLE PUBLICATIONS PVT LTD
Page : 146 pages
File Size : 52,6 Mb
Release : 2020-08-15
Category : Biography & Autobiography
ISBN : 8210379456XXX

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Civil Services Chronicle September 2020 by Mr. NN OJha Pdf

The No.1 Magazine for IAS Aspirants Since 1990

Nuclear Reactions of Astrophysical Interest

Author : Scilla Degl’Innocenti,Livio Lamia,Rosario Gianluca Pizzone
Publisher : Frontiers Media SA
Page : 248 pages
File Size : 47,9 Mb
Release : 2021-07-29
Category : Science
ISBN : 9782889711192

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Nuclear Reactions of Astrophysical Interest by Scilla Degl’Innocenti,Livio Lamia,Rosario Gianluca Pizzone Pdf

Astronomy Reports

Author : Anonim
Publisher : Unknown
Page : 492 pages
File Size : 49,8 Mb
Release : 1999
Category : Astronomy
ISBN : CHI:53765056

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Astronomy Reports by Anonim Pdf

Origin and Evolution of the Elements: Volume 4, Carnegie Observatories Astrophysics Series

Author : Andrew McWilliam,Michael Rauch
Publisher : Cambridge University Press
Page : 520 pages
File Size : 40,8 Mb
Release : 2004-09-23
Category : Science
ISBN : 0521755786

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Origin and Evolution of the Elements: Volume 4, Carnegie Observatories Astrophysics Series by Andrew McWilliam,Michael Rauch Pdf

This Carnegie volume discusses the origin and evolution of elements in our galaxy and others.

From Lithium to Uranium (IAU S228)

Author : International Astronomical Union. Symposium
Publisher : Cambridge University Press
Page : 648 pages
File Size : 46,5 Mb
Release : 2005
Category : Science
ISBN : 0521851998

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From Lithium to Uranium (IAU S228) by International Astronomical Union. Symposium Pdf

Proceedings of IAU S228 detailing progress in our knowledge of element production and evolution.

Light Elements in the Universe (IAU S268)

Author : International Astronomical Union. Symposium
Publisher : Cambridge University Press
Page : 528 pages
File Size : 40,9 Mb
Release : 2010-05-13
Category : Science
ISBN : 0521765064

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Light Elements in the Universe (IAU S268) by International Astronomical Union. Symposium Pdf

IAU Symposium 268 presents an overview of the most recent observational and theoretical research on the formation and evolution of light elements in the Universe: H, He, Li, Be, B, and their isotopes. Astrophysicists from a variety of subfields discuss recent developments that will improve our understanding of the light elements and provide important clues to stellar and galactic evolution, Big Bang nucleosynthesis, and cosmology. Striking observational progress has been achieved recently through the advent of next generation ground- and space-based telescopes, such as the cosmic microwave background experiments that allow the accurate determination of the baryon density of the Universe. New theoretical breakthroughs in describing stellar interiors and the chemical evolution of complex systems and the remaining challenges in this field are also addressed. This critical review is a useful resource for all those interested in the chemical evolution of the Universe.

Literature 1997, Part 1

Author : Astronomisches Rechen-InstitutARI
Publisher : Springer Science & Business Media
Page : 1746 pages
File Size : 48,8 Mb
Release : 2013-11-11
Category : Science
ISBN : 9783642517587

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Literature 1997, Part 1 by Astronomisches Rechen-InstitutARI Pdf

Astronomy and Astrophysics Abstracts is devoted to the recording, summarizing and indexing of astronomical publications throughout the world. Two volumes are scheduled to appear per year. Volume 67 records 10,903 papers covering besides the classical fields of astronomy and astrophysics such matters as space flights related to astronomy, lunar and planetary probes and satellites, meteorites and interplanetary matter, X rays and cosmic rays, quasars and pulsars. The abstracts are classified under more than one hundred subject categories thus permitting quick surveying of the bulk of material published on the same topic within six months. For instance, this volume records 119 papers on minor planets, 155 papers on supernovae, and 554 papers on cosmology.

Astrophysics and Space Science

Author : L.B.F.M. Waters,C. Waelkens,Karel A. van der Hucht,P.A. Zaal
Publisher : Springer Science & Business Media
Page : 562 pages
File Size : 44,7 Mb
Release : 1998-08-31
Category : Science
ISBN : 0792351525

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Astrophysics and Space Science by L.B.F.M. Waters,C. Waelkens,Karel A. van der Hucht,P.A. Zaal Pdf

This conference proceedings contains review papers and contributed papers discussing early results from the Infrared Space Observatory (ISO) on the subject of stellar evolution. Three topics have been emphasized in the book: young stellar objects and Vega-type stars, circumstellar matter of massive stars, and late stages of stellar evolution. The very rich harvest of new results from ISO is demonstrated by the many discoveries of new solid state and molecular bands in the spectra of stars and circumstellar shells, and by spectacular images of circumstellar and interstellar matter. The book is intended for professional astronomers and students.

Stars as Laboratories for Fundamental Physics

Author : Georg G. Raffelt
Publisher : University of Chicago Press
Page : 692 pages
File Size : 41,9 Mb
Release : 1996-05
Category : Science
ISBN : 0226702723

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Stars as Laboratories for Fundamental Physics by Georg G. Raffelt Pdf

Much of what we know about neutrinos is revealed by astronomical observations, and the same applies to the axion, a conjectured new particle that is a favored candidate for the main component of the dark matter of the universe.