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Bogdan, Akos (2010): X-ray emission from nearby early-type galaxies and origin of Type Ia Supernovae. Dissertation, LMU München: Fakultät für Physik

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Figure

Figure 1.1: Modern classification scheme of Supernovae, taken from Turatto (2003). Note, that Type IaSupernovae are the result of thermonuclear explosions of white dwarf stars, whereas other Supernovaeoriginate from the compact iron core collapse in massive evolved stars.
Figure 1.2: Light curves of nearby SNe Ia (Perlmutter, 2003). On the upper panel their absolute magnitudeis plotted against the decay time
Figure 1.3: Hubble diagram for 42 high redshift and 18 low redshift SNe Ia, taken from Perlmutter et al.(1999)
Figure 1.4: The fate of an accreting carbon-oxygen white dwarf as a function of their initial mass (MC+O)and accretion rate ( M˙) (Nomoto & Kondo, 1991)
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