The Carbon Star Phenomenon

Author:   Robert F. Wing
Publisher:   Springer
Edition:   2000 ed.
Volume:   177
ISBN:  

9780792363477


Pages:   616
Publication Date:   31 July 2000
Format:   Paperback
Availability:   In Print   Availability explained
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The Carbon Star Phenomenon


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Overview

The atmospheres of many stars have chemical compositions that are significantly different from that of the interstellar medium from which they are formed. This symposium considered all kinds of late-type stars showing altered compositions, the carbon stars being simply the best-known of these. All stages of stellar evolution from the main sequence to the ejection of a planetary nebula were considered, with emphasis on the changes that occur on the asymptotic giant branch. The spectroscopic properties of the photospheres and circumstellar envelopes of chemically-peculiar red giant stars, their origins via single-star evolution or mass transfer in binary systems, and the methods currently used to study them in 2000 were all discussed in detail. This volume includes the full texts of papers given orally at the symposium and abstracts of the posters.

Full Product Details

Author:   Robert F. Wing
Publisher:   Springer
Imprint:   Springer
Edition:   2000 ed.
Volume:   177
Dimensions:   Width: 16.00cm , Height: 3.30cm , Length: 24.00cm
Weight:   1.990kg
ISBN:  

9780792363477


ISBN 10:   0792363477
Pages:   616
Publication Date:   31 July 2000
Audience:   College/higher education ,  Professional and scholarly ,  Postgraduate, Research & Scholarly ,  Professional & Vocational
Format:   Paperback
Publisher's Status:   Active
Availability:   In Print   Availability explained
This item will be ordered in for you from one of our suppliers. Upon receipt, we will promptly dispatch it out to you. For in store availability, please contact us.

Table of Contents

Preface. Tribute to Nuzhet Gokdogammaan. Conference photo. List of participants. Introduction. Session I - Surveys. Session II - Models and Abundance Determinations. Session III - Observed Spectra and Energy Distributions. Session IV - Variability. Session V - Post-AGB Stars. Session VI - Binarity. Session VII - Mass-Loss, Winds, and Formation of Dust Grains. Session VIII - Circumstellar Shells. Session IX - Circumstellar Emission and Environment. Session X - Nucleosynthesis and Evolution. Session XI - Galactic Chemical Evolution. Session XII - Observing Facilities. Abstracts of Posters. Indexes.

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