Примеры использования Luminous stars на Английском языке и их переводы на Русский язык
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The most luminous stars in the Galaxy and the Magellanic Clouds.
NGC 2363-V1 is one of the most luminous stars known.
These luminous stars have been used as standard candle distance indicators.
AG Carinae List of most luminous stars Cutri, R. M. 2003.
All three components of δ Circini A are hot luminous stars.
This star is among the most luminous stars in the Milky Way.
On average it has an absolute magnitude of -9.5, making it visually one of the most luminous stars known.
It surrounds one of the most luminous stars known, the Pistol Star. .
It is classified as a luminous blue variable and is one of the most luminous stars known.
These luminous stars can be detected at great distances, and are then used to extend the distance scale to nearby galaxies in the Local Group.
It is a blue supergiant,one of the most luminous stars in the Milky Way.
Note that even the most luminous stars are much less luminous than the more luminous persistent extragalactic objects, such as quasars.
A distance of 5 kpc and a bolometric magnitude of -9.4 put HR Car among the most luminous stars of the galaxy.
It is a Luminous Blue Variable and one of the most luminous stars known, but so far away that it is invisible to the naked eye.
AFGL 2298 has an absolute bolometric magnitude of -11.25,making it one of the most luminous stars known.
Many of the hottest and most luminous stars known are luminous blue variables and other early-type stars. .
Had the latter distance been correct, Canopus would have been one of the most luminous stars in the Milky Way galaxy.
The bias towards luminous stars when observing a patch of sky affects calculations of the average absolute magnitude and average distance to a group of stars. .
Case(2) applies to a stellar system composed entirely of luminous stars i.e. no dark matter or black holes.
It is also one of the most luminous stars known in the Galaxy, with an estimated bolometric luminosity of around 850,000 times that of the Sun and a radius 103 times that of the Sun.
The outer galaxy is relatively bright and contains many luminous stars indicative of star formation.
This allows almost the entire energy output of the system to be observed at wavelengths that are not strongly affected by interstellar extinction,leading to estimates of the luminosity that are more accurate than for other extremely luminous stars.
Other studies have estimated ages up to 2 million years, butthe existence of the most massive and luminous stars provide a hard upper limit of 2.5 million years on the possible age.
Because of the luminous stars that are at a further distance, it will appear as if our sample of stars is farther away than it actually is, and that each star is intrinsically brighter than it actually is.
It is estimated at 2 million times as luminous as the sun which makes it one of the most luminous stars in the galaxy.
The project is aimed at investigating the photometric variations of massive luminous stars by using two Austrian nanosatellites(BRITE-Austria and UniBRITE) that observe on two different wavelengths.
All five Wolf Rayets are extremely young massive objects with OIf*/WN spectral types, amongst the most luminous stars in the galaxy.
It has long been suspected that this is due to colliding winds in a close pair of hot luminous stars, but investigations have failed to show any significant radial velocity variations to support this.
The Pistol Star, a luminous blue variable is 1.6 million times brighter than the Sun making it one of the most luminous stars in the Milky Way.
NML Cygni was discovered in 1965 by Neugebauer, Martz, and Leighton who described two extremely red luminous stars, their colour being consistent with a black body temperature of 1,000 K. The name NML comes from the names of these three discoverers.