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On the Formation of the Most Massive Stars in the Galaxy

  • Roberto J. Galván-Madrid

Part of the Springer Theses book series (Springer Theses)

Table of contents

  1. Front Matter
    Pages i-xiii
  2. Roberto Galván-Madrid
    Pages 1-13
  3. Roberto Galván-Madrid
    Pages 15-38
  4. Roberto Galván-Madrid
    Pages 39-72
  5. Roberto Galván-Madrid
    Pages 103-103
  6. Back Matter
    Pages 105-122

About this book

Introduction

The most massive stars in the galaxy - those with more than 15 to 20 solar masses - are lilkely to ionize their surroundings before they reach their final mass. How can they accrete in spite of the presence of over-pressurized gas?

This thesis presents results of Submillimeter Array (SMA) and Very Large Array (VLA) studies of massive star formation regions in the early stages of ionization, as well as an analysis of numerical simulations of the evolution of these young HII regions. The results favor a picture in which very massive stars form in accretion flows that are partially ionized and that keep accreting material from their environment.

The American Astronomical Society selected Roberto Galvan-Madrid as a prize winner for The Rodger Doxsey Travel Prize in 2010.

Keywords

Accretion flow Accretion signifiers Gravitational collapse HII regions Ionization stages Jets and outflows Massive star formation Springer astronomy thesis Submillimeter array Ultracompact HII regions Very large array

Authors and affiliations

  • Roberto J. Galván-Madrid
    • 1
  1. 1.AstrophysicsHarvard-Smithsonian CenterCambridgeUSA

Bibliographic information

  • DOI https://doi.org/10.1007/978-1-4614-3308-8
  • Copyright Information Springer Science+Business Media New York 2012
  • Publisher Name Springer, New York, NY
  • eBook Packages Physics and Astronomy
  • Print ISBN 978-1-4614-3307-1
  • Online ISBN 978-1-4614-3308-8
  • Series Print ISSN 2190-5053
  • Series Online ISSN 2190-5061
  • Buy this book on publisher's site