「super-giant」の共起表現(1語右で並び替え)

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共起表現

「super-giant」の共起表現一覧(1語右で並び替え)

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The F-type	supergiant also forms a binary system with an unseen st
A blue	supergiant, Aludra has only been around a fraction of t
It is a yellow	supergiant and is a pulsating variable known as a RV Ta
It is a yellow	supergiant and is the prototype of a class of pulsating
a spectroscopic binary with a yellow G-type	supergiant and a white A-type main sequence dwarf.
NGC 4889, also known as Caldwell 35, is a	supergiant class-4 elliptical galaxy, the brightest wit
etion of matter from the stellar wind of the	supergiant companion.
leagues to investigate the conditions inside	supergiant exoplanets.
high mass, the star will expand into a blue	supergiant in the next few million years and eventually
PV Telescopii is a class B-type (blue)	supergiant in the constelation Telescopium.
star designation of ADS 10611, in which the	supergiant is orbited by a dwarf companion once every f
At a separation of 32.6 arcseconds from the	supergiant is an 11th magnitude neighbour.
A yellow-white	supergiant, it lies around 590 light years from Earth a
Being a blue	supergiant, it is destined to become a red supergiant i
HR Carinae is a	supergiant, luminous blue variable star located in the
us member is the ~2nd magnitude white-yellow	supergiant Mirfak, also known as Alpha Persei.
close binary, comprising Alnitak Aa (a blue	supergiant of spectral and luminosity type O9.7 Ibe, wi
Lambda Velorum is a	supergiant or bright giant star of spectral class K5.
6 Cassiopeiae (6 Cas) is an A type bright	supergiant or hypergiant.
star that may have already passed through a	supergiant phase and is now contracting and heating up
VX Sagittarii is a late-type red	supergiant star (likely even a red hypergiant) located
ted with the Uhuru source 4U 0900-40 and the	supergiant star HD 77581.
Omicron Draconis (ο Dra, ο Draconis) is a	supergiant star in the constellation Draco located 322.
hin the next few million years expand into a	supergiant star before ending its life in a spectacular
a remnant or gas cloud illuminated by nearby	supergiant star Rigel in Orion.
4U 0900-40, and which is associated with the	supergiant star HD 77581.
Z Capricorni (Z Cap) is a M-type	supergiant star in the constellation of Capricornus.
HD 115337 is a red or yellow	supergiant star in the constellation Camelopardalis.
86 Gm - Diameter of Rigel, a blue	supergiant star (largest star on right)
Mu Normae is a blue	supergiant star in the constellation Norma.
Australis is a yellow-white bright giant or	supergiant star in the southern constellation of Triang
Although ζ Ophiuchi is a hot blue	supergiant star it appears reddish due to interstellar
Sanduleak -69° 202a was a magnitude 12 blue	supergiant star, located on the outskirts of the Tarant
It is fairly average for an orange	supergiant star, well into the later stages of its stel
may not be suited for life, because it is a	supergiant star, spectral type F7Ib.
R Coronae Borealis is a yellow	supergiant star, and is the prototype of the RCB class
constellation, γ Velorum, is a bright 1.75m	supergiant star.
element helium, and transferring into a red	supergiant star.
They are	supergiant stars of spectral types B or A. Variations i
Due to limb darkening, all giant and	supergiant stars present unique challenges when measuri
me comes from the fact it has five prominent	supergiant stars residing in it.
large cluster of new stars containing 14 red	supergiant stars was discovered there and named RSGC1.
	Supergiant stars use up their hydrogen "fuel" much fast
Blue and red	supergiant stars, star clusters, and star-forming regio
han 20 million years old and contains 26 red	supergiant stars, the largest grouping of such stars kn
t is one of the most luminous stars known, a	supergiant that has used up the hydrogen fuel in its co
e variable, from F-type to G-type and from a	supergiant to a bright giant.
Nu-2 Sagittarii A is a spectral type K1	supergiant which has an apparent magnitude of +5.00.
Xi-1 Sagittarii is a spectral type B9.5	supergiant which has an apparent magnitude of +5.08.
Pismis 24-1SW is a very bright blue	supergiant, which probably is about to become a luminou
or that ruse again and it is unlikely a blue	supergiant will be available again given their rarity.
and Plez's study), the star is a normal red	supergiant, with a radius around 600 solar radii.
mponent ζ Capricorni A being a yellow G-type	supergiant with an apparent magnitude of +3.77.
osion of a massive star, most probably a red	supergiant with a helium core which had lost almost all
Eta Leonis is a white	supergiant with the stellar classification A0Ib.
Iota¹ Scorpii is a yellow-white F-type	supergiant with an apparent magnitude of +3.02.
119 Tauri is a M-type red	supergiant with a mean apparent magnitude of +4.32.
29 Canis Majoris is an O-type blue	supergiant with a mean apparent magnitude of +4.88.
ο1 Canis Majoris is an orange K-type	supergiant with a mean apparent magnitude of +3.89.
l Carinae is a yellow G-type	supergiant with a mean apparent magnitude of +3.69.
ο1 Centauri is a yellow G-type	supergiant with a mean apparent magnitude of +5.07.
P Carinae is a white A-type	supergiant with a mean apparent magnitude of +4.65.
ο2 Centauri is a white A-type	supergiant with a mean apparent magnitude of +5.12.
ψ1 Aurigae is an orange K-type	supergiant with a mean apparent magnitude of +4.92.
V533 Carinae is a white A-type	supergiant with a mean apparent magnitude of +4.59.
Theta Arae is a blue-white B-type	supergiant with an apparent magnitude of +3.65.
Nu Aquilae is a yellow-white F-type	supergiant with an apparent magnitude of +4.64.
σ Canis Majoris is an orange K-type	supergiant with a mean apparent magnitude of +3.49.
Iota² Scorpii is a white A-type	supergiant with an apparent magnitude of +4.78.
HD 125288 is a blue-white B-type	supergiant with an apparent magnitude of +4.30.
κ Cassiopeiae is a blue-white B-type	supergiant with a mean apparent magnitude of +4.17.
oscopic binary classified as a yellow G-type	supergiant with an apparent magnitude of +5.09.
onent, b Velorum A, is a yellow-white F-type	supergiant with a mean apparent magnitude of +3.77.
ta Trianguli Australis A, is a yellow G-type	supergiant with an apparent magnitude of +3.86.
anis Majoris is classified as an O-type blue	supergiant with a mean apparent magnitude of +4.37.
eta Arae is an orange K-type bright giant or	supergiant with an apparent magnitude of +2.84.
CS Camelopardalis A, is a blue-white B-type	supergiant with a mean apparent magnitude of 4.21m.
mponent, α¹ Capricorni A, is a yellow G-type	supergiant with an apparent magnitude of +4.30.
y which is classified as a blue-white B-type	supergiant with an apparent magnitude of +4.71.

共起表現

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