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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.
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