「main sequence」の共起表現(1語右で並び替え)

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共起表現

「main sequence」の共起表現一覧(1語右で並び替え)

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n years, it will soon evolve away from the	main-sequence and expand to become a red giant.
most cataclysmic variables, matter from a	main-sequence companion star is gravitationally stripped
core of a star that reached the end of its	main-sequence life cycle, ejected most of its outer laye
times that of the Sun, the star spent its	main-sequence life as an A-type star.
surface in a fraction of an A-type star's	main-sequence lifetime, where they can be observed as fi
WASP-11/HAT-P-10 is a magnitude-12	main-sequence orange dwarf star about 400 light years aw
although they are common in a group of dim	main-sequence, reddish M dwarfs known as flare stars.
an extrasolar planet orbiting an ordinary	main-sequence star (51 Pegasi).
Astronomers categorize it as a	main-sequence star of spectral class K2, which means the
An A-type	main-sequence star (A V) is a main-sequence (hydrogen-bu
An F-type	main-sequence star (F V) is a main-sequence, hydrogen-fu
HD 36960 (HR 1887) is a B-type	main-sequence star in the constellation Orion.
It is a yellow	main-sequence star of spectral type G3.
Pi Ceti is a blue	main-sequence star located about 440 light-years from Ea
wn as COROT-Exo-4) is a yellow-white dwarf	main-sequence star in the constellation Monoceros.
HD 154857 is a yellow	main-sequence star approximately 224 light years away in
HD 50554 is a yellow-white	main-sequence star [F8V] that currently fuse hydrogen in
HIP 14810 is a G-type	main-sequence star located approximately 170 light-years
HD 89307 is a yellow	main-sequence star located approximately 108 light-years
HD 49674 is an 8th magnitude G-type	main-sequence star (spectral type G5V) located approxima
approximately 86.29 ly from Earth and is a	main-sequence star of the spectral type G and luminosity
It is a white	main-sequence star with strengthened H and K lines of Ca
HD 136118 is a F-type	main-sequence star located approximately 171 light-years
consisting of two main components: a blue	main-sequence star of class B0.5V and a magnitude of 2.9
tates that the companion may be a "bloated	main-sequence star, possibly still filling its Roche Lob
It is an F-type	main-sequence star, a type of hydrogen-fusing star that
ed that it was a B-type star when it was a	main-sequence star.
asses, it was an A-type star when it was a	main-sequence star.
warf, a low-mass helium star or an evolved	main-sequence star.
Only a few	main-sequence stars have revealed warm (>120 K) zodiacal
White dwarfs arise from the cores of	main-sequence stars and are therefore very hot when they
llar system containing one of the smallest	main-sequence stars whose radius has been measured.
llar system containing one of the smallest	main-sequence stars whose radius has been measured.
he dust that orbits around several hundred	main-sequence stars is cold and comes from a Kuiper-belt
air Regulus B and Regulus C, which are dim	main-sequence stars.
When it was	main-sequence, the spectral type was early F or late A.
lsar planets found around PSR B1257+12 and	main-sequence yellow dwarf 51 Pegasi.

共起表現

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「main sequence」の共起表現一覧(1語右で並び替え)