Book contents
- Frontmatter
- Contents
- Preface to the first edition
- Preface to the second edition
- Acknowledgments
- 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
- Appendix 1 Basic hydrodynamic and MHD equations
- Appendix 2 Jeans masses and fragmentation
- Appendix 3 Basic radiative transfer
- List of symbols
- Bibliography
- Index
Preface to the second edition
Published online by Cambridge University Press: 30 October 2009
- Frontmatter
- Contents
- Preface to the first edition
- Preface to the second edition
- Acknowledgments
- 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
- Appendix 1 Basic hydrodynamic and MHD equations
- Appendix 2 Jeans masses and fragmentation
- Appendix 3 Basic radiative transfer
- List of symbols
- Bibliography
- Index
Summary
Initially it seemed like a good idea to revise this book, because so much has been learned about star and planet formation over the last ten years. It eventually became clear that it was a bad idea to revise this book, because so much has been learned about star and planet formation over the last ten years. By then I was halfway through and it was too late to back out.
I therefore beg the reader's indulgence for things I have left out or treated schematically. At some point in a project like this “the best is the enemy of the good”, as Voltaire apparently said; just give up and send it off. Perhaps there is some value in having a treatment that does not try to cover everything in an enormous tome, but instead provides accessible points of departure. As was the case for the first version, I hope that this will be a useful reference for non-specialists as well as a starting point for researchers entering the field.
- Type
- Chapter
- Information
- Accretion Processes in Star Formation , pp. xiiiPublisher: Cambridge University PressPrint publication year: 2008