Book contents
- Frontmatter
- Contents
- Participants
- Preface
- History of the Local Group
- Primordial nucleosynthesis
- Galactic structure
- The Large Magellanic Cloud: Structure and kinematics
- The Local Group as an astrophysical laboratory for massive star feedback
- Hot gas in the Local Group and low-redshift intergalactic medium
- Stages of satellite accretion
- The star formation history in the Andromeda halo
- Bulge populations in the Local Group
- The Local Group as a laboratory for the chemical evolution of galaxies
- Massive stars in the Local Group: Star formation and stellar evolution
- Massive Young Clusters in the Local Group
- Magellanic Cloud planetary nebulae as probes of stellar evolution and populations
- The old globular clusters: Or, life among the ruins
- Chemical evolution models of Local Group galaxies
Participants
Published online by Cambridge University Press: 12 May 2010
- Frontmatter
- Contents
- Participants
- Preface
- History of the Local Group
- Primordial nucleosynthesis
- Galactic structure
- The Large Magellanic Cloud: Structure and kinematics
- The Local Group as an astrophysical laboratory for massive star feedback
- Hot gas in the Local Group and low-redshift intergalactic medium
- Stages of satellite accretion
- The star formation history in the Andromeda halo
- Bulge populations in the Local Group
- The Local Group as a laboratory for the chemical evolution of galaxies
- Massive stars in the Local Group: Star formation and stellar evolution
- Massive Young Clusters in the Local Group
- Magellanic Cloud planetary nebulae as probes of stellar evolution and populations
- The old globular clusters: Or, life among the ruins
- Chemical evolution models of Local Group galaxies
Summary
- Type
- Chapter
- Information
- The Local Group as an Astrophysical LaboratoryProceedings of the Space Telescope Science Institute Symposium, held in Baltimore, Maryland May 5–8, 2003, pp. vii - xPublisher: Cambridge University PressPrint publication year: 2006