The Life and Death of StarsCambridge University Press, 25 de mar. de 2013 In this well-illustrated text, Kenneth R. Lang explains the life cycle of stars, from the dense molecular clouds that are stellar nurseries to the enigmatic nebulae some stars leave behind in their violent ends. Free of mathematical equations and technical jargon, Lang's lively and accessible text provides physical insights into how stars such as our Sun are born, what fuels them and keeps them bright, how they evolve and the processes by which they eventually die. The book demonstrates the sheer scope and variety of stellar phenomena in the context of the universe as a whole. Boxed focus elements enhance and amplify the discussion for readers looking for more depth. Featuring more than 150 figures, including color plates, The Life and Death of Stars is a modern and up-to-date account of stars written for a broad audience, from armchair astronomers and popular science readers to students and teachers of science. |
Conteúdo
18 | |
Atomic and Subatomic Particles | 31 |
Transmutation of the Elements | 58 |
What Makes the Sun Shine? | 76 |
The Extended Solar Atmosphere | 102 |
Comparisons of the Sun with Other Stars | 128 |
The Lives of Stars | 157 |
The Material Between the Stars | 186 |
Stellar End States | 219 |
A Larger Expanding Universe | 259 |
Birth Life and Death of the Universe | 287 |
Quotation References 3 13 | 313 |
319 | |
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alpha particle angular astronomer big bang bright carbon cloud collapse confirmed convective core coronal coronal loops cosmic dark deflected denoted detected diagram distance dust Earth Earth’s atmosphere electrical electrons elements emitted energy equator expanding explosion fi‘om Figure first flow galaxies giant stars gravitational heat helium Hubble Hubble Space Telescope hydrogen hydrogen atoms infrared inside intense interstellar invisible ionized known light-years located luminosity luminous magnetic field main sequence main-sequence stars massive stars material measurements Milky million molecules Moon motion moving nearby neutrinos neutron star nuclear reactions nucleus Observatory observed orbital outer photosphere physicist planet pressure produced protons pull pulsar radiation radio radioactive radius rays red giant regions rotation satellites shine solar flares solar masses solar wind Space Telescope spectral lines spectrum speed of light star’s stellar subatomic sufficiently sunspots supergiant supernova thermal universe velocity wavelengths waves white dwarf white dwarf star x-ray