pair-instability supernova oor Sjinees
pair-instability supernova
Vertalings in die woordeboek Engels - Sjinees
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It is thought that SN 2006gy is a likely candidate for a pair-instability supernova.
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Another hypothesis is the pulsational pair-instability supernova, a massive star that may lose about half its mass before a series of violent pulses begins.
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In explosions of very large stars (250 or more times the mass of the Sun), such as pair-instability supernovae, photodisintegration is a major factor in the supernova event.
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Pair-instability supernovae can only happen in stars with a mass range from around 130 to 250 solar masses and low to moderate metallicity (low abundance of elements other than hydrogen and helium – a situation common in Population III stars).
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A star with 140 M☉ ≲ Mms ≲ 300 M☉ explodes because of the energy consumption arising from an electron-positron pair-production instability during the static O-burning stage, and is referred to as a pair-instability supernova (PISN).
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5 sinne gevind in 4 ms. Hulle kom uit baie bronne en word nie nagegaan nie.