Very Low-Mass Stars and Brown Dwarfs
Title | Very Low-Mass Stars and Brown Dwarfs PDF eBook |
Author | Rafael Rebolo |
Publisher | Cambridge University Press |
Pages | 284 |
Release | 2000-11-27 |
Genre | Science |
ISBN | 9780521663359 |
This volume provides a state-of-the-art review of our current knowledge of brown dwarfs and very low-mass stars. The hunt for and study of these elusive objects is currently one of the most dynamic areas of research in astronomy for two reasons. Brown dwarfs bridge the gap between stars and planets, and they may constitute an important part of the 'dark matter' of the Universe. This volume presents review articles from a team of international authorities who gathered at a conference in La Palma to assess the spectacular progress that has been made in this field in the last few years.
New Light on Dark Stars
Title | New Light on Dark Stars PDF eBook |
Author | Neill I. Reid |
Publisher | Springer Science & Business Media |
Pages | 492 |
Release | 2013-11-27 |
Genre | Science |
ISBN | 1447136632 |
Perhaps the most common question that a child asks when he or she sees the night sky from a dark site for the first time is: 'How many stars are there?' This happens to be a question which has exercised the intellectual skills of many astronomers over the course of most of the last century, including, for the last two decades, one of the authors of this text. Until recently, the most accurate answer was 'We are not certain, but there is a good chance that almost all of them are M dwarfs. ' Within the last three years, results from new sky-surveys - particularly the first deep surveys at near infrared wavelengths - have provided a breakthrough in this subject, solidifying our census of the lowest-mass stars and identifying large numbers of the hitherto almost mythical substellar-mass brown dwarfs. These extremely low-luminosity objects are the central subjects of this book, and the subtitle should be interpreted accordingly. The expression 'low-mass stars' carries a wide range of meanings in the astronomical literature, but is most frequently taken to refer to objects with masses comparable with that of the Sun - F and G dwarfs, and their red giant descendants. While this definition is eminently reasonable for the average extragalactic astronomer, our discussion centres on M dwarfs, with masses of no more than 60% that of the Sun, and extends to 'failed stars' - objects with insufficient mass to ignite central hydrogen fusion.
A Search for Pulsation in Young Brown Dwarfs and Very Low Mass Stars
Title | A Search for Pulsation in Young Brown Dwarfs and Very Low Mass Stars PDF eBook |
Author | Ann Marie Cody |
Publisher | Universal-Publishers |
Pages | 318 |
Release | 2013-08 |
Genre | Science |
ISBN | 1612334210 |
In 2005, Palla & Baraffe proposed that brown dwarfs and very low mass stars (
New Light on Dark Stars
Title | New Light on Dark Stars PDF eBook |
Author | Neil Reid |
Publisher | Springer |
Pages | 560 |
Release | 2009-09-02 |
Genre | Science |
ISBN | 9783540808404 |
There has been very considerable progress in research into low-mass stars, brown dwarfs and extrasolar planets during the past few years, particularly since the fist edtion of this book was published in 2000. In this new edtion the authors present a comprehensive review of both the astrophysical nature of individual red dwarf and brown dwarf stars and their collective statistical properties as an important Galactic stellar population. Chapters dealing with the observational properies of low-mass dwarfs, the stellar mass function and extrasolar planets have been completely revised. Other chapters have been significantly revised and updated as appropriate, including important new material on observational techniques, stellar acivity, the Galactic halo and field star surveys. The authors detail the many discoveries of new brown dwarfs and extrasolar planets made since publication of the first edition of the book and provide a state-of-the-art review of our current knowledge of very low-mass stars, brown dwarfs and extrasolar planets, including both the latest observational results and theoretical work.
Rotation Studies of Young Very Low Mass Stars and Brown Dwarfs
Title | Rotation Studies of Young Very Low Mass Stars and Brown Dwarfs PDF eBook |
Author | María Victoria Rodríguez-Ledesma |
Publisher | |
Pages | 104 |
Release | 2009 |
Genre | |
ISBN |
Very Low Mass Stars and Brown Dwarfs in Galactic Clusters
Title | Very Low Mass Stars and Brown Dwarfs in Galactic Clusters PDF eBook |
Author | Nigel Charles Hambly |
Publisher | |
Pages | |
Release | 1991 |
Genre | Brown dwarf stars |
ISBN |
New Light on Dark Stars
Title | New Light on Dark Stars PDF eBook |
Author | I. Neill Reid |
Publisher | |
Pages | 470 |
Release | 2000 |
Genre | Astronomy |
ISBN | 9781447136651 |
Perhaps the most common question that a child asks when he or she sees the night sky from a dark site for the first time is: 'How many stars are there?' This happens to be a question which has exercised the intellectual skills of many astronomers over the course of most of the last century, including, for the last two decades, one of the authors of this text. Until recently, the most accurate answer was 'We are not certain, but there is a good chance that almost all of them are M dwarfs. ' Within the last three years, results from new sky-surveys - particularly the first deep surveys at near infrared wavelengths - have provided a breakthrough in this subject, solidifying our census of the lowest-mass stars and identifying large numbers of the hitherto almost mythical substellar-mass brown dwarfs. These extremely low-luminosity objects are the central subjects of this book, and the subtitle should be interpreted accordingly. The expression 'low-mass stars' carries a wide range of meanings in the astronomical literature, but is most frequently taken to refer to objects with masses comparable with that of the Sun - F and G dwarfs, and their red giant descendants. While this definition is eminently reasonable for the average extragalactic astronomer, our discussion centres on M dwarfs, with masses of no more than 60% that of the Sun, and extends to 'failed stars' - objects with insufficient mass to ignite central hydrogen fusion.