Book contents
- Frontmatter
- Contents
- Participants
- Preface
- High-mass star formation by gravitational collapse of massive cores
- Observations of massive-star formation
- Massive-star formation in the Galactic center
- An x-ray tour of massive-star-forming regions with Chandra
- Massive stars: Feedback effects in the local universe
- The initial mass function in clusters
- Massive stars and star clusters in the Antennae galaxies
- On the binarity of Eta Carinae
- Parameters and winds of hot massive stars
- Unraveling the Galaxy to find the first stars
- Optically observable zero-age main-sequence O stars
- Metallicity-dependent Wolf-Rayet winds
- Eruptive mass loss in very massive stars and Population III stars
- From progenitor to afterlife
- Pair-production supernovae: Theory and observation
- Cosmic infrared background and Population III: An overview
Participants
Published online by Cambridge University Press: 04 August 2010
- Frontmatter
- Contents
- Participants
- Preface
- High-mass star formation by gravitational collapse of massive cores
- Observations of massive-star formation
- Massive-star formation in the Galactic center
- An x-ray tour of massive-star-forming regions with Chandra
- Massive stars: Feedback effects in the local universe
- The initial mass function in clusters
- Massive stars and star clusters in the Antennae galaxies
- On the binarity of Eta Carinae
- Parameters and winds of hot massive stars
- Unraveling the Galaxy to find the first stars
- Optically observable zero-age main-sequence O stars
- Metallicity-dependent Wolf-Rayet winds
- Eruptive mass loss in very massive stars and Population III stars
- From progenitor to afterlife
- Pair-production supernovae: Theory and observation
- Cosmic infrared background and Population III: An overview
Summary
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- Type
- Chapter
- Information
- Massive StarsFrom Pop III and GRBs to the Milky Way, pp. vii - viiiPublisher: Cambridge University PressPrint publication year: 2009