Tidal Evolution and Oscillations in Binary Stars
Author : Antonio Claret
Publisher :
Page : 360 pages
File Size : 19,70 MB
Release : 2005
Category : Science
ISBN :
Author : Antonio Claret
Publisher :
Page : 360 pages
File Size : 19,70 MB
Release : 2005
Category : Science
ISBN :
Author : International Astronomical Union. Symposium
Publisher : Cambridge University Press
Page : 524 pages
File Size : 40,26 MB
Release : 2007-08-27
Category : Science
ISBN : 9780521863483
IAU S240 focuses on recent advances across the broad field of binary star research.
Author : C. Aerts
Publisher : Springer Science & Business Media
Page : 872 pages
File Size : 44,22 MB
Release : 2010-01-19
Category : Science
ISBN : 1402058039
Understanding the stars is the bedrock of modern astrophysics. Stars are the source of life. The chemical enrichment of our Milky Way and of the Universe withallelementsheavierthanlithiumoriginatesintheinteriorsofstars.Stars arethe tracersofthe dynamics ofthe Universe,gravitationallyimplying much more than meets the eye. Stars ionize the interstellar medium and re-ionized the early intergalactic medium. Understanding stellar structure and evolution is fundamental. While stellar structure and evolution are understood in general terms, we lack important physical ingredients, despite extensive research during recent decades.Classicalspectroscopy,photometry,astrometryandinterferometryof stars have traditionally been used as observational constraints to deduce the internal stellar physics. Unfortunately, these types of observations only allow the tuning of the basic common physics laws under stellar conditions with relatively poor precision. The situation is even more worrisome for unknown aspects of the physics and dynamics in stars. These are usually dealt with by using parameterised descriptions of, e.g., the treatments of convection, rotation,angularmomentumtransport,theequationofstate,atomicdi?usion andsettlingofelements,magneto-hydrodynamicalprocesses,andmore.There is a dearth of observational constraints on these processes, thus solar values areoftenassignedtothem.Yetitishardtoimaginethatonesetofparameters is appropriate for the vast range of stars.
Author : WasaburÅ Unno
Publisher :
Page : 442 pages
File Size : 36,26 MB
Release : 1989
Category : Oscillations
ISBN :
Author : Andrzej S. Baran
Publisher : Frontiers Media SA
Page : 178 pages
File Size : 19,28 MB
Release : 2021-10-13
Category : Science
ISBN : 2889714772
Author : Giacomo Beccari
Publisher : Cambridge University Press
Page : 359 pages
File Size : 32,34 MB
Release : 2019-04-18
Category : Science
ISBN : 1108428584
An advanced review of how binary stars affect stellar evolution, presenting results from state-of-the art models and recent observations.
Author : Swetlana Hubrig
Publisher : Springer Science & Business Media
Page : 304 pages
File Size : 18,96 MB
Release : 2007-10-13
Category : Science
ISBN : 3540747451
This volume presents results from the ESO workshop Multiple Stars across the H-R Diagram, held in Garching in July 2005. It covers observations of multiple stars from ground and space, dynamical and stellar evolution in multiple systems, formation and early evolution of multiple stars, and special components of multiple stars. The book reviews the current state of observational and theoretical knowledge and discusses future studies for further progress in the field.
Author : Alvaro Gimenez
Publisher : Springer Science & Business Media
Page : 349 pages
File Size : 30,30 MB
Release : 2007-04-05
Category : Science
ISBN : 1402050275
This book is the proceedings of an international conference entitled "Close Binaries in the 21st Century: New Opportunities and Challenges", held in Syros island, Greece, June 27-30, 2005. The papers collected in this volume detail the latest achievements in the field and reflect the state of the art of the dynamically evolving area of binary star research.
Author : Dirk Brouwer
Publisher : Elsevier
Page : 611 pages
File Size : 10,32 MB
Release : 2013-09-03
Category : Science
ISBN : 148322578X
Methods of Celestial Mechanics provides a comprehensive background of celestial mechanics for practical applications. Celestial mechanics is the branch of astronomy that is devoted to the motions of celestial bodies. This book is composed of 17 chapters, and begins with the concept of elliptic motion and its expansion. The subsequent chapters are devoted to other aspects of celestial mechanics, including gravity, numerical integration of orbit, stellar aberration, lunar theory, and celestial coordinates. Considerable chapters explore the principles and application of various mathematical methods. This book is of value to mathematicians, physicists, astronomers, and celestial researchers.
Author : National Research Council
Publisher : National Academies Press
Page : 324 pages
File Size : 29,75 MB
Release : 2011-02-04
Category : Science
ISBN : 0309157994
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.