How supernovae explode, and get their brightness
13 years, 7 months ago

How supernovae explode, and get their brightness

The Hindu  

Scientists have made an important step toward understanding the details of how Type Ia supernovae explode and the origin of their immense luminosity. The widely accepted theory is that Type Ia supernovae are thermonuclear explosions of a white dwarf star in a close binary system. Now, a team of researchers has examined new and detailed observations of 41 of these objects and concluded that there are clear signatures of gas outflows from the supernova ancestors, which do not appear to be white dwarfs "If the star system originally contained two white dwarfs before the supernova, then there shouldn’t be any sodium,” remarked Nidia Morrell of the Carnegie Observatories. The astronomers also ruled out other possible sources of the sodium absorption features including interstellar clouds or a galactic—scale wind blown by the host galaxy. "Typically, gas with these characteristics is attributed to the stellar wind blown by red giant companion stars, not white dwarfs,” he concluded.

History of this topic

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