Thermonuclear SupernovaeP. Ruiz-Lapuente, R. Canal, J. Isern Springer Science & Business Media, 6 груд. 2012 р. - 890 стор. All theoretical and observational topics relevant to the understanding of the thermonuclear (Type Ia) supernova phenomenon are thoroughly and consistently reviewed by a panel including the foremost experts in the field. The book covers all aspects, ranging from the observations of SNe Ia at all stages and all wavelengths to the 2D and 3D modelling of thermonuclear flames in very dense plasmas. Scenarios for close binary evolution leading to SNe Ia are discussed. Particular emphasis is placed on the homogeneity vs. diversity of SNe Ia and on their use as standard candles to measure cosmological parameters. The book reflects the recent and very significant progress made in both the modelling of the explosions and in the observational field. |
Зміст
SCENARIOS | 31 |
an overview W Hillebrandt | 33 |
OBSERVED SPECTRA AND LIGHT CURVES | 122 |
Modeling the light curves of Type Ia supernovae W D Vacca | 137 |
Luminous supersoft Xray sources as Type la progenitors | 163 |
A phenomenological approach to the formation of massive CO white | 177 |
on the binary progenitors and expected statistics | 205 |
The elusive close binary white dwarfs A Bragaglia et al | 229 |
biases and uncertainties E Cappellaro | 647 |
Statistical studies of supernovae O S Bartunov D Yu Tsvetkov | 732 |
supernova subclasses A V Filippenko | 795 |
models and spectra S E Woosley | 821 |
common envelope evolution | 839 |
New perspectives on Type Ic supernovae A Clocchiatti | 863 |
CONCLUDING REMARKS | 884 |
STATISTICS CONSTRAINTS ON PROGENITORS | 349 |
Інші видання - Показати все
Загальні терміни та фрази
accretion rate Arnett Astron Astrophys binary bolometric burning front C+O WD calculations carbon carbon detonation Chandrasekhar mass convective core deflagration degenerate delayed detonation density detonation model disk distance distribution ejecta electron capture emission energy equation evolution explosion Figure Filippenko flame flux fraction galaxies H II regions Hamuy helium Höflich Hubble hydrodynamic Iben ignition initial instability Isern Khokhlov Kirshner layers Leibundgut light curves Livio Livne luminosity magnitude mass loss mass transfer massive maximum light merging Mochkovitch neutrino neutron star Nomoto observed obtained opacity optical optical depth parameters peak phase Phillips photons photosphere Physics progenitors propagation radiation radius redshift region Roche lobe Ruiz-Lapuente scale scenario simulations SNe Ia spectra spectrum spiral arms star formation stellar sub-Ch sub-Chandrasekhar Suntzeff temperature thermal Thermonuclear Supernovae Thielemann turbulent Tutukov Type Ia supernovae wavelength Wheeler white dwarf Woosley & Weaver Yungelson