Примеры использования Spectral type на Английском языке и их переводы на Русский язык
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The star is thought to be about 7 times more luminous than the Sun. γ2 Delphini is an orange subgiant star of spectral type"K1IV" and an apparent magnitude of 4.27.
The spectral type is now,
Its spectral type is A1p;
It is an orange dwarf(spectral type K1 V),
distance, spectral type, right ascension/ declination, etc.
orbits Nu Scorpii A. It has an apparent magnitude of 5.40, but its spectral type is unknown.
The secondary star(designated as HD 178911 B) has an apparent magnitude of 6.74 and a spectral type of G1V, which is very similar to our Sun at a distance of 160 light years.
age, spectral type, and Teff are similar to the well-studied planet β Pictoris b.
Mitchella is an assumed stony S-type asteroid, which is also the overall spectral type for members of the Flora family.
infrared spectra features can be matched by a star of spectral type M5III.
They are main-sequence stars of spectral type B2 to B9(3 to 9 times as massive as the Sun)
Using the more modern revised Morgan-Keenan scheme, a spectral type of C-N5- C2 6- has been published,
γ1 Delphini is a yellow-white dwarf star of spectral type"F7V" and an apparent magnitude of 5.14.
This composite spectral type indicates young very massive hydrogen-burning stars that are just starting to convect nitrogen
although it is unclear what the temperature or spectral type of the underlying star actually is,
XX Per is a red supergiant of spectral type M4Ib with an effective temperature of 3,700 K. It has a large infrared excess,
The primary is a red giant of spectral type M0III, a star that has used up its core hydrogen,
The 1890 eruption may have been fairly typical of LBV eruptions, with an early F spectral type, and it has been estimated that the star may currently have an opaque stellar wind forming a pseudo-photosphere with a temperature of 9,000 K-14,000 K which would be typical for an LBV in eruption.
CK Carinae is a red supergiant of spectral type M3.5Iab with an effective temperature of 3,550 K. It is one of the largest stars,
It is composed of two ageing orange giants of spectral types K0III and K2III.