Book contents
- Frontmatter
- Contents
- List of Boxes
- List of Figures
- List of Tables
- Preface
- 1 History and development
- 2 Stars
- 3 Variable stars
- 4 Rotating variable stars
- 5 Eclipsing variable stars
- 6 Pulsating variable stars
- 7 Eruptive variable stars
- 8 Pre-main-sequence variable stars
- 9 Miscellaneous variable stars
- 10 Epilogue
- Appendix: Acronyms
- References
- Resources
- Index
Preface
Published online by Cambridge University Press: 28 October 2009
- Frontmatter
- Contents
- List of Boxes
- List of Figures
- List of Tables
- Preface
- 1 History and development
- 2 Stars
- 3 Variable stars
- 4 Rotating variable stars
- 5 Eclipsing variable stars
- 6 Pulsating variable stars
- 7 Eruptive variable stars
- 8 Pre-main-sequence variable stars
- 9 Miscellaneous variable stars
- 10 Epilogue
- Appendix: Acronyms
- References
- Resources
- Index
Summary
The roots of this book go back over forty years. As an undergraduate in 1960, I was exposed to the variable star research at the David Dunlap Observatory of the University of Toronto. Mentors such as Don Fernie, Jack Heard, and Helen Sawyer Hogg brought the field to life. As a graduate student, I sampled both theory (with Pierre Demarque) and observation (with Don Fernie). Then I was fortunate to obtain a faculty position at the University of Toronto's brand-new Erindale Campus in Mississauga, west of Toronto. I was concerned with teaching, supervising students, and building a new university campus.
My research continued, and my graduate teaching responsibility was a course on variable stars. This book evolved from that course. The 1970s were in many ways the ‘golden age’ of variable stars at the University of Toronto. A dozen graduate students undertook M.Sc. and/or Ph.D. these on variable stars. The David Dunlap Observatory, being a ‘local’ observatory under our control, enabled both large-scale surveys, and long-term studies to be carried out – both of which are almost impossible at modern-day national observatories. The observatory was equipped with both a 1.88m spectroscopic telescope, and 0.6m and 0.5m photometric telescopes, and many of these thesis projects combined these techniques in a very effective way. I learned much from these graduate students, and owe much to my colleagues, including a succession of Directors of the David Dunlap Observatory – who were also Chairs of the Department of Astronomy and Astrophysics.
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- Chapter
- Information
- Understanding Variable Stars , pp. xviii - xxiiPublisher: Cambridge University PressPrint publication year: 2007