Приклади вживання Massive star Англійська мовою та їх переклад на Українською
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Colloquial
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Ecclesiastic
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Computer
Some suspect the Big Bang was actually a massive star going supernova,
which forms as soon as a massive star becomes supernova,
About 10,000 years ago, the supernova that created the nebular remnant CTB 1 not only destroyed a massive star but blasted its newly formed neutron star core-- a.
The resulting remnant would be a black hole since it is highly unlikely such a massive star could ever lose sufficient mass for its core not to exceed the limit for a neutron star. .
The Orion Nebula is the nearest region of massive star formation to Earth, and is therefore studied
there is a massive star cluster R136 with the biggest
a 20.5 solar mass(M☉), slightly evolved hot massive star with a radius of 12 R☉ and spectral type O6-7 II-III.
Astronomers think massive star formation must require some sort of additional triggering mechanism,
Previously, it was thought that that the less massive star in a binary system acts as a“vampire”,
computer modeling suggests that near the Central black hole of our galaxy- Sagittarius A*- can be a very massive star that every 10 thousand years is approaching very close to the hole,
In the favored scenario of a massive star collapse(sometimes known as a collapsar) the week-long burst of optical/infrared emission
It turns out that neutrons can also obey the exclusion principle and neutrons will be produced in abundance when a massive star collpses, but even neutron degeneracy cannot stop the collapse of massive stars--- anything over 3 to 5 solar masses cannot be stopped, it will become a black hole according to current thinking.
But a supernova is when you have a pretty massive star, and its core is collapsing,
as core collapse supernovae.[27][28] In the pre-supernova massive star this includes helium burning, carbon burning,
Avi Loeb has theorised that if a massive star is rapidly rotating,
possibly the remnant of a massive star cluster that has been stripped down by the Galactic Center.
sufficiently old for a massive star to evolve away from the main sequence
The most massive stars evolve most rapidly.
More massive stars will evolve even more quickly.
More massive stars die by photodisintegration.