Book contents
- Frontmatter
- Contents
- Preface
- Conference participants
- Conference photograph / poster
- 1 Physics of H2 and HD
- Astrophysical Importance of H2
- Radiative and Electronic Excitation of Lyman and Werner Transitions in H2
- The Cooling of Astrophysical Media by H2 and HD
- Highly Excited Singlet Ungerade States of H2 and their Theoretical Description
- Laboratory Studies of Long-range Excited States of H2
- A Model of Interstellar Dark Matter
- Mass of H2 Dark Matter in the Galactic Halo
- 2 Formation - Destruction
- 3 Observations and Models
- 4 Extragalactic and Cosmology
- 5 Outlook
- Author index
Mass of H2 Dark Matter in the Galactic Halo
from 1 - Physics of H2 and HD
Published online by Cambridge University Press: 04 August 2010
- Frontmatter
- Contents
- Preface
- Conference participants
- Conference photograph / poster
- 1 Physics of H2 and HD
- Astrophysical Importance of H2
- Radiative and Electronic Excitation of Lyman and Werner Transitions in H2
- The Cooling of Astrophysical Media by H2 and HD
- Highly Excited Singlet Ungerade States of H2 and their Theoretical Description
- Laboratory Studies of Long-range Excited States of H2
- A Model of Interstellar Dark Matter
- Mass of H2 Dark Matter in the Galactic Halo
- 2 Formation - Destruction
- 3 Observations and Models
- 4 Extragalactic and Cosmology
- 5 Outlook
- Author index
Summary
- Type
- Chapter
- Information
- Molecular Hydrogen in Space , pp. 57 - 60Publisher: Cambridge University PressPrint publication year: 2000