The Origin of StarsWhere do stars come from and how do they form? These are profound questions which link the nature of our Universe to the roots of mankind. Yet, until a recent revolution in understanding, the proposed answers have been raw speculation. Now, accompanying penetrating observations, a new picture has come into prominence.This book presents the latest astounding observations and scientific ideas covering star formation, star birth and early development. It encompasses all aspects, from the dramatic stories of individual objects, to the collective influence of entire stellar systems.The very first stars to come into existence and the nurturing of planets are discussed to provide the reader with a comprehensive overview. Presenting background information with only the essential mathematics, this book will appeal to scientists wishing to expand their horizons, students seeking solid foundations, and general readers with enquiring minds. |
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Contents
| 1 | |
| 9 | |
| 31 | |
| 53 | |
| 69 | |
| 87 | |
The Magnetic Mediation | 101 |
The Birth | 119 |
The Young Stars | 139 |
Jets and Outflows | 161 |
Massive Stars | 185 |
The Distributions | 201 |
Cosmological Star Formation | 221 |
Epilogue | 237 |
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Common terms and phrases
accretion angular momentum appear associated atomic become called central Class classical close clumps clusters collapse collisions consistent contain cores cosmic rays critical dense density detected determine diffusion direction disk dispersion distribution dust dynamical effect emission energy envelope evidence evolution evolve expected flow force fragmentation Galactic galaxies given gravitational heating hydrogen increase indicate infall infrared initial ionisation jets lines locations luminosity magnetic field mass massive stars material means measured mechanism medium molecular clouds molecules motions objects observed occurs optical origin outflows phase physical predicted present pressure produced protostar protostellar radiation range reached regions remains require result rotation scale shock sources speed stage star formation stellar stellar winds strong structure sufficient suggest surface temperature theory thermal turbulence typical Universe wavelengths waves wide wind young stars




