Stellar StructureUniversity of Chicago Press, 1965 - 648 pagine |
Dall'interno del libro
45 pagine corrispondenti a perturbation in questo libro
Dov'è il resto di questo libro?
Risultati 1-3 di 45
Sommario
Introduction | 1 |
Nuclear Abundances | 23 |
The Problem of the Nuclei of D He³ Li Be and | 60 |
Copyright | |
52 sezioni non visualizzate
Altre edizioni - Visualizza tutto
Parole e frasi comuni
absorption abundance approximation assumed atoms beta decay bound-free Burbidge calculations Cameron Chandrasekhar chemical composition clusters Coma Cluster computed considered constant conv convective zone core cross-section degeneracy density diagram discussed effect elements emission energy equation equilibrium evolutionary explosion formula Fowler fraction free-free galaxies Gaunt factors given gm/cm³ gravitational Greenstein He¹ He³ helium Hoyle HR diagram hydrogen hydrostatic equilibrium increase instability ionization isotopes km/sec layers light-curves lines of force luminosity magnetic field magnitude main sequence main-sequence mass maximum Mestel neutrino neutrons novae nuclear reactions nuclei observed obtained opacity oscillations particles perturbation photon Phys pressure radiation radiative radius ratio red giant region rotation s-process Sandage scattering Schatzman Schwarzschild sequence solar spectra spectrum star stellar evolution Strömgren supernovae of type surface Table temperature theory thermal tion velocity virial theorem white dwarf