Our systems are now restored following recent technical disruption, and we’re working hard to catch up on publishing. We apologise for the inconvenience caused. Find out more

Recommended product

Popular links

Popular links


Accretion Processes in Star Formation

Accretion Processes in Star Formation

Accretion Processes in Star Formation

2nd Edition
Lee Hartmann, University of Michigan, Ann Arbor
November 2008
Available
Paperback
9780521531993
AUD$136.32
exc GST
Paperback
USD
eBook

    Our understanding of the formation of stars and planetary systems has changed greatly since the first edition of this book was published. This new edition has been thoroughly updated, and now includes material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF), disk evolution and planet formation. This book provides a comprehensive picture of the formation of stars and planetary systems, from their beginnings in cold clouds of molecular gas to their emergence as new suns with planet-forming disks. At each stage gravity induces an inward accretion of mass, and this is a central theme for the book. The author brings together current observations, rigorous treatments of the relevant astrophysics, and 150 illustrations, to clarify the sequence of events in star and planet formation. It is a comprehensive account of the underlying physical processes of accretion for graduate students and researchers.

    • Includes new material on molecular clouds, binaries, star clusters and the stellar initial mass function (IMF), disk evolution and planet formation
    • Brings together current observations, astrophysics and 150 illustrations to clarify the sequence of events in star and planet formation
    • Presents a complete picture of the formation of stars and planetary systems, from their beginnings in cold clouds of molecular gas to their emergence as new suns with planet-forming disks

    Product details

    November 2008
    Paperback
    9780521531993
    346 pages
    247 × 176 × 17 mm
    0.7kg
    60 b/w illus.
    Available

    Table of Contents

    • 1. Overview
    • 2. Beginnings: molecular clouds
    • 3. Initial conditions for protostellar collapse
    • 4. Protostellar cloud collapse
    • 5. Protostellar collapse: observations vs theory
    • 6. Binaries, clusters, and the IMF
    • 7. Disk accretion
    • 8. The disks of pre-main sequence stars
    • 9. The FU Orionis objects
    • 10. Disk winds, jets, and magnetospheric accretion
    • 11. Disk accretion and early stellar evolution
    • 12. Disk evolution and planet formation
    • Appendixes
    • References
    • Index.
      Author
    • Lee Hartmann , University of Michigan, Ann Arbor

      Lee Hartmann is currently Professor of Astronomy at the University of Michigan and a vice-president of the American Astronomical Society. He is an expert on star formation and protoplanetary disk evolution.