Примеры использования Solar masses на Английском языке и их переводы на Русский язык
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A nuclear ring of active star formation has been found in the center with a rate of formation greater than 100 solar masses per year.
Type Ia supernova progenitors are white dwarf stars that are close to the Chandrasekhar limit of about 1.44 solar masses and are accreting matter from a binary companion star.
Ground-based detectors could potentially detect binaries containing an intermediate mass black hole of several hundred solar masses.
somewhere between 0.6 and 12× 1016 solar masses M⊙.
in nearby galaxies are suspected to be IMBHs, with masses of a hundred to a thousand solar masses.
When the white dwarf approaches the Chandrasekhar limit of 1.4 solar masses(M☉), it may explode as a Type Ia supernova.
The stellar mass of Antlia Dwarf is estimated to be about 2-4×106 solar masses, while its total mass(within the visible radius) is approximately 4× 107 solar masses.
The neon-burning process(nuclear decay) is a set of nuclear fusion reactions that take place in massive stars at least 8 Solar masses.
are extraordinarily massive, with several million solar masses(M☉) and multiple stellar populations.
The black hole was estimated to be between 2 and 5 billion solar masses.
The measurements have so far failed to detect any neutral hydrogen in it-the upper limit is just 600 solar masses.
Measurements have so far failed to detect neutral hydrogen in it-the upper limit is 466 solar masses.
containing several solar masses of gas, are expelled at huge speeds into interstellar space.
Its radius is around 20 times that of the latter, with a mass that has been estimated to be between 45 and 60 solar masses.
the mass of the compact object is only a few solar masses.
For the hypernova SN 2006gy, studies indicate that perhaps 40 solar masses of the original star were released as Ni-56, almost the entire mass of the star's core regions.
The estimated mass of the cluster is 450,000 solar masses, suggesting it will likely become a globular cluster in the future.
Both the high luminosity and slow decay indicate that the supernova's progenitor was a star with an initial mass as high as 250 solar masses.
The entire mass of the star is ejected, so a nebular remnant is produced and many solar masses of heavy elements are returned to interstellar space.
gas with the mass of about 2.8× 105 solar masses, which is three times more than the mass of the stars in this galaxy.