Observer’s Guide to Stellar Evolution: The Birth, Life and Death of Stars: The Patrick Moore Practical Astronomy Series
Autor Mike Inglisen Limba Engleză Paperback – 6 noi 2002
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Specificații
ISBN-13: 9781852334659
ISBN-10: 1852334657
Pagini: 260
Ilustrații: XVII, 238 p.
Dimensiuni: 155 x 235 x 14 mm
Greutate: 0.5 kg
Ediția:Softcover reprint of the original 1st ed. 2003
Editura: SPRINGER LONDON
Colecția Springer
Seria The Patrick Moore Practical Astronomy Series
Locul publicării:London, United Kingdom
ISBN-10: 1852334657
Pagini: 260
Ilustrații: XVII, 238 p.
Dimensiuni: 155 x 235 x 14 mm
Greutate: 0.5 kg
Ediția:Softcover reprint of the original 1st ed. 2003
Editura: SPRINGER LONDON
Colecția Springer
Seria The Patrick Moore Practical Astronomy Series
Locul publicării:London, United Kingdom
Public țintă
Popular/generalCuprins
A Brief Introduction.- 1 Stellar Evolution — The Basics.- 1.1 Distance to the Stars.- 1.2 The Nearest Stars.- 1.3 The Brightness and Luminosity of Stars.- 1.4 The Magnitudes of Stars.- 1.5 The Brightest Stars.- 1.6 The Colour of Stars.- 1.7 The Size and Mass of Stars.- 1.8 The Biggest Stars.- 1.9 The Constituents of Stars.- 1.10 The Spectra of Stars.- 1.11 Stellar Classification.- 1.12 The Hertzsprung—Russell Diagram.- 1.13 The H—R Diagram and a Star’s Radius.- 1.14 The H—R Diagram and a Star’s Luminosity.- 1.15 The H—R Diagram and a Star’s Mass.- 2 Beginnings — Star Birth.- 2.1 Introduction.- 2.2 The Interstellar Medium.- 2.3 Nebulae.- 2.4 Molecular Clouds.- 2.5 Protostars.- 2.6 Pre-Main Sequence Evolution.- 2.7 Mass Loss and Mass Gain.- 2.8 Star Clusters.- 2.9 Stellar Associations and Streams.- 2.10 Star Formation Triggers.- 3 The Main Sequence and Beyond.- 3.1 Introduction.- 3.2 Our Nearest Star — The Sun.- 3.3 From the Surface to the Core.- 3.4 The Proton—Proton Chain.- 3.5 The Flow of Energy from the Core to the Surface.- 3.6 Main Sequence Lifetimes.- 3.7 Towards the Red Giant.- 3.8 Helium Burning and the Helium Flash.- 3.9 Red Giants, Star Clusters and the H—R Diagram.- 3.10 Post-Main Sequence Star Clusters: The Globular Clusters.- 3.11 Stars That Pulsate.- 3.12 Cepheid Variables and the Period—Luminosity Relationship.- 3.13 Cepheid Variables: Temperature and Mass.- 3.14 RR Lyrae and Long-Period Variable Stars.- 4 The End Point — Star Death.- 4.1 Introduction.- 4.2 The Asymptotic Giant Branch.- 4.3 Dredge-Ups.- 4.4 Mass Loss and Stellar Winds.- 4.5 Infrared Stars.- 4.6 The End of an AGB Star’s Life.- 4.7 Planetary Nebulae.- 4.8 White Dwarf Stars.- 4.9 Electron Degeneracy and White Dwarfs.- 4.10 The Chandrasekhar Limit.- 4.11 WhiteDwarf Evolution.- 4.12 White Dwarf Origins.- 4.13 High-Mass Stars: Nuclear Burning and an Onion.- 4.14 Iron, Supernovae and the Formation of the Elements.- 4.15 The Supernova Remnant.- 4.16 A Final Note on Supernovae.- 4.17 Neutron Stars, Pulsars and Black Holes.- 4.18 From Beginning to End.- Appendix 1 Degeneracy.- Appendix 2 Books, Magazines and Organizations.- Appendix 3 The Greek Alphabet.- Appendix 4 Colour Photographs.- Object Index.
Caracteristici
Introduces the theory of stellar evolution through practical observation of stars Accessible to every amateur astronomer, regardless of background knowledge Mathematics is not ignored, but is presented in 'boxes' that readers can skip over if they prefer Includes supplementary material: sn.pub/extras