Skip to main content

Mass Loss and Evolution of O-Type Stars

  • Book
  • © 1979

Overview

Part of the book series: International Astronomical Union Symposia (IAUS, volume 83)

This is a preview of subscription content, log in via an institution to check access.

Access this book

eBook USD 16.99 USD 39.99
Discount applied Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 54.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access

Licence this eBook for your library

Institutional subscriptions

Table of contents (67 chapters)

  1. Optical Spectroscopy

  2. U.V. Spectroscopy

Keywords

About this book

The organization of this Symposium had its beginnings at the International Astronomical Union General Assembly in Grenoble in 1976. The initial "rounding up" of the Scienti­ fic Organizing Committee was begun by Drs. Snow and Swings; most of us who became the eventual organizing committee met a few times during the Assembly and formulated the essential outlines of the meeting. Extensive correspondence with all the committee subsequently established the program. The idea was to bring together both observers and theoreticians to discuss the stellar winds and mass loss rates and their effects on evolutions of O-type stars. On the observational side, there are now spectroscopic data from the far UV to the near IR regions concerning the stellar winds. There is also information about the free-free emission in the wind from the IR and radio portions of the spectrum. Fortunately, these different detection methods give more or less the same mass loss rate for the one star, s Pup" which has been observed at all wavelengths. One of the intents of the first three sessions of this Symposium is to outline the eXisting data on mass loss rates as it per­ tains to the O-type stars.

Editors and Affiliations

  • Joint Institute for Laboratory Astrophysics, University of Colorado, Boulder, USA

    P. S. Conti

  • Astrophysical Institute, Vrije Universiteit, Brussels, Belgium

    C. W. H. Loore

Bibliographic Information

  • Book Title: Mass Loss and Evolution of O-Type Stars

  • Editors: P. S. Conti, C. W. H. Loore

  • Series Title: International Astronomical Union Symposia

  • DOI: https://doi.org/10.1007/978-94-009-9452-2

  • Publisher: Springer Dordrecht

  • eBook Packages: Springer Book Archive

  • Copyright Information: International Astronomical Union 1979

  • Hardcover ISBN: 978-90-277-0988-2Due: 31 May 1979

  • Softcover ISBN: 978-90-277-0989-9Published: 31 May 1979

  • eBook ISBN: 978-94-009-9452-2Published: 06 December 2012

  • Series ISSN: 1743-9213

  • Series E-ISSN: 2352-2186

  • Edition Number: 1

  • Number of Pages: 520

  • Topics: Astronomy, Observations and Techniques

Publish with us