Catalogue of star clusters and associations. Suppl. 1 : Pt. A. Introduction
Author : J. Ruprecht
Publisher :
Page : 120 pages
File Size : 34,92 MB
Release : 1981
Category : Stars
ISBN :
Author : J. Ruprecht
Publisher :
Page : 120 pages
File Size : 34,92 MB
Release : 1981
Category : Stars
ISBN :
Author : BASU, BAIDYANATH
Publisher : PHI Learning Pvt. Ltd.
Page : 599 pages
File Size : 48,71 MB
Release : 2010-01-01
Category : Science
ISBN : 812034071X
This invaluable book, now in its second edition, covers a wide range of topics appropriate for both undergraduate and postgraduate courses in astrophysics. The book conveys a deep and coherent understanding of the stellar phenomena, and basic astrophysics of stars, galaxies, clusters of galaxies and other heavenly bodies of interest. Since the first appearance of the book in 1997, significant progress has been made in different branches of Astronomy and Astrophysics. The second edition takes into account the developments of the subject which have taken place in the last decade. It discusses the latest introduction of L and T dwarfs in the Hertzsprung-Russel diagram (or H-R diagram). Other developments discussed pertain to standard solar model, solar neutrino puzzle, cosmic microwave background radiation, Drake equation, dwarf galaxies, ultra compact dwarf galaxies, compact groups and cluster of galaxies. Problems at the end of each chapter motivate the students to go deeper into the topics. Suggested readings at the end of each chapter have been complemented.
Author : M. A. C. Perryman
Publisher : Cambridge University Press
Page : 695 pages
File Size : 25,46 MB
Release : 2009
Category : Nature
ISBN : 0521514894
An authoritative account of the contributions to science made by the Hipparcos satellite, for astronomers, astrophysicists and cosmologists.
Author : Albrecht Unsöld
Publisher : Springer Science & Business Media
Page : 586 pages
File Size : 42,65 MB
Release : 2001
Category : Science
ISBN : 9783540678779
This new edition of the classic textbook The New Cosmos presents a comprehensive introductory survey of the whole field of astronomy and astrophysics. Among the topics covered are: - Classical astronomy and the Solar System - Instruments and observational methods - The Sun and the stars - The Milky Way and other galaxies - Cosmology - The origin of the Solar System - The evolution of the Earth and of life The observational methods and results of astronomical research as well as their theoretical foundations and interrelations are presented in an understandable format. The rapid progress of observational techniques and of theoretical understanding in the past decade are introduced and summarized in this timely and readable volume. This revised and extended new printing demonstrates the rapid advances in astronomical research and observation in the three years since the appearance of the 5th edition. The most important new results can be found within, providing in particular up-to-date information on our solar system, neutrino radiation from the Sun, the farthest galaxies and quasars and the development of the Universe.
Author : S. Böhme
Publisher : Springer Science & Business Media
Page : 787 pages
File Size : 18,82 MB
Release : 2013-12-14
Category : Science
ISBN : 3662123347
Astronomy and Astrophysics Abstracts, which has appeared in semi-annual volumes since 1969, is devoted to the recording, summarizing and indexing of astronomical publications throughout the world. It is prepared under the auspices of the International Astronomical Union (according to a resolution adopted at the 14th General Assembly in 1970). Astronomy and Astrophysics Abstracts aims to present a comprehensive documenta tion of literature in all fields of astronomy and astrophysics. Every effort will be made to ensure that the average time interval between the date of receipt of the original literature and publication of the abstracts will not exceed eight months. This time interval is near to that achieved by monthly abstracting journals, compared to which our system of accumu lating abstracts for about six months offers the advantage of greater convenience for the user. Volume 31 contains literature published in 1982 and received before July 15, 1982; some older literature which was received late and which is not recorded in earlier volumes is also included. We acknowledge with thanks contributions to this volume by Dr. J. Bouska, Prague, who surveyed journals and publications in Czech and supplied us with abstracts in English .
Author : A.B. Underhill
Publisher : Springer Science & Business Media
Page : 295 pages
File Size : 44,98 MB
Release : 2012-12-06
Category : Science
ISBN : 9401035563
At this time when astronomers are being surprised by the discovery of objects which emit a fabulously large amount of energy, that is the quasi-stellar radio sources and the quasi-stellar galaxies, and when by the means of space vehicles X rays, gamma rays and cosmic rays are being observed to come from the depths of interstellar space, one may ask why write a book about stars. Stars seem to be almost incidental when one looks at the universe in terms of exceedingly great energies. Nevertheless, stars exist. They are accessible to study and they have not yet revealed all their secrets. This is enough to arouse interest and to cause one to try to find answers to the questions which arise. The early type stars are particularly interesting because they are spendthrift stars pouring out their energy at a great rate. But their brilliance is also their undoing. They must evolve rather quickly, on an astrophysical scale. Thus by studying these stars we are studying a population in change. The implications from the local and from the cosmological viewpoint are important if one wishes to understand the details of stellar evolution and of galactic structure. Perhaps one of the simplest reasons for writing a book about the early type stars is to see if some of the conundrums pre sented by the spectra of these stars can be unravelled when all the available infor mation is brought together.
Author : International Astronomical Union. Symposium
Publisher : Cambridge University Press
Page : 606 pages
File Size : 10,56 MB
Release : 2010-02-04
Category : Science
ISBN : 9780521764995
Star clusters are important to many areas of astronomy, and as the basic building blocks of galaxies, they can be used as key diagnostic tools within a wide range of disciplines in astrophysics. Star cluster populations are powerful tracers of the formation, assembly and evolutionary history of their parent galaxies. Although their importance has been recognised for decades, only in recent years has this area seen a major investment in time and effort. IAU Symposium 266 consolidates the expertise of leading researchers from a variety of topical subfields in astrophysics, to provide a comprehensive presentation of cutting-edge developments in theory, observations and simulations of star clusters and star cluster systems across a range of sizes and epochs. This volume gives an account of this forefront research, answering fundamental questions that will improve our understanding of numerous related issues and show how this field will take its next major step forward.
Author : Cathie Clarke
Publisher : Springer
Page : 356 pages
File Size : 48,2 MB
Release : 2015-09-11
Category : Science
ISBN : 3662472902
Where do most stars (and the planetary systems that surround them) in the Milky Way form? What determines whether a young star cluster remains bound (such as an open or globular cluster), or disperses to join the field stars in the disc of the Galaxy? These questions not only impact understanding of the origins of stars and planetary systems like our own (and the potential for life to emerge that they represent), but also galaxy formation and evolution, and ultimately the story of star formation over cosmic time in the Universe. This volume will help readers understand our current views concerning the answers to these questions as well as frame new questions that will be answered by the European Space Agency's Gaia satellite that was launched in late 2013. The book contains the elaborated notes of lectures given at the 42nd Saas-Fee Advanced Course “Dynamics of Young Star Clusters & Associations" by Cathie Clarke (University of Cambridge) who presents the theory of star formation and dynamical evolution of stellar systems, Robert Mathieu (University of Wisconsin) who discusses the kinematics of star clusters and associations, and I. Neill Reid (S pace Telescope Science Institute) who provides an overview of the stellar populations in the Milky Way and speculates on from whence came the Sun. As part of the Saas-Fee Advanced Course Series, the book offers an in-depth introduction to the field serving as a starting point for Ph.D. research and as a reference work for professional astrophysicists.
Author : International Astronomical Union. Symposium
Publisher : Springer Science & Business Media
Page : 438 pages
File Size : 31,48 MB
Release : 1990-06-30
Category : Science
ISBN : 9780792307716
Some 70 papers present the flare star problem from both a physical and evolutionary aspect, and represent an interaction between investigators working on flare stars in clusters and associations, and those working on the UV Ceti stars in solar vicinity. The variety of perspectives reveal a physical similarity among several non-stable phenomena, and suggest that the different manifestations of stellar activity result from the release of some unknown kind of energy in the outer layers of young stars. The papers deal not only with different aspects of flare stars, but also with such related objects as T Tauri stars, fluors, and Herbig-Haro objects. Annotation copyrighted by Book News, Inc., Portland, OR
Author : Steven Stahler
Publisher : Springer
Page : 205 pages
File Size : 45,33 MB
Release : 2017-11-04
Category : Science
ISBN : 3319228013
All stars are born in groups. The origin of these groups has long been a key question in astronomy, one that interests researchers in star formation, the interstellar medium, and cosmology. This volume summarizes current progress in the field, and includes contributions from both theorists and observers. Star clusters appear with a wide range of properties, and are born in a variety of physical conditions. Yet the key question remains: How do diffuse clouds of gas condense into the collections of luminous objects we call stars? This book will benefit graduate students, newcomers to the field, and also experienced scientists seeking a convenient reference.