Примеры использования Main sequence на Английском языке и их переводы на Русский язык
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the outer envelope expanded to many times the radius it possessed as a main sequence star.
is a star in the stage when it has not yet reached the main sequence.
have been identified by studying color-color outliers in cases where one member is off the main sequence.
is a yellow G-type main sequence dwarf with a mean apparent magnitude of +5.63.
late A type main sequence stars, and typical brightness fluctuations are 0.1 magnitudes with periods on the order of one day.
The instability strip intersects the main sequence in the region of A and F stars(1-2 solar mass(M☉))
colour-colour diagram to calibrate the absolute magnitudes of the stars, for example fitting the main sequence or identifying features such as a horizontal branch,
now formally known as the main sequence; and giants.
will remain on the main sequence for hundreds of billions of years
meaning that there is agreement in identifying it as a main sequence star more luminous
The presence of significant amounts of dust around the star implies a young age of the system and led to debate about whether it had joined the main sequence or was still a pre-main sequence star However, when the star's
a 60 M☉ star, has experienced a relatively brief LBV stage after it left the main sequence, and is now losing the last of its hydrogen before becoming a more conventional Wolf-Rayet star.
Nearly all stars on the main sequence are X-ray emitters.
HD 69830 is a main sequence star of spectral type G8V.
It is a blue-white main sequence star of apparent magnitude 5.21.
Luyten's Star is a medium-sized red dwarf star on the main sequence.
B Cephei B is a magnitude 7.8 A2 main sequence star 13.6" distant.
Fitting the main sequence, and pre-main sequence gives a cluster age of 1 million years or less.
Primary component A is a main sequence star with a stellar classification of F8V.
It is a stage that follows the main sequence for low- to intermediate-mass stars.