Modelling the diversity of spectra and light curves of thermonuclear supernovae
Description preview
Type Ia supernovae are bright astrophysical transients that are understood to be caused by thermonuclear explosions of white dwarf stars in binaries. White dwarfs are remnants left behind when low-mass stars reach the end of their lives, and so these explosions are a key aspect of stellar evolution. The extreme conditions in thermonuclear…
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