「yellow-white」の共起表現一覧(1語右で並び替え)
該当件数 : 96件
The face is | yellow-white and the underparts are barred black and yel |
instars grow to about 5 cm (2.0 in) and are | yellow-white and black banded with yellow spots around e |
2 G. Trianguli Australis is a | yellow-white bright giant or supergiant star in the sout |
Epsilon Cephei is a | yellow-white, Delta Scuti variable star, located about 8 |
Nu2 Columbae is a | yellow-white dwarf star in the constellation Columba. |
WASP-3 is a magnitude 10 | yellow-white dwarf star located about 727 light-years aw |
HD 40979 is a | yellow-white dwarf star about 109 light-years away in th |
OROT-4 (formerly known as COROT-Exo-4) is a | yellow-white dwarf main-sequence star in the constellati |
hat 14 Andromedae was formerly a white or a | yellow-white dwarf star early in its life. |
HD 231701 is a | yellow-white dwarf star approximately 354 light years aw |
94 Ceti A is a | yellow-white dwarf star with about 1.3 times the mass of |
HD 200156 is a | yellow-white dwarf with a spectral type of F5V and is ap |
φ² Pavonis), also known as HD 196378, is a | yellow-white dwarf star approximately 82 light-years awa |
ar, this class of star may also be termed a | yellow-white dwarf. |
Upsilon Aquarii is a | yellow-white F-type subgiant with an apparent magnitude |
Iota¹ Scorpii is a | yellow-white F-type supergiant with an apparent magnitud |
Delta Volantis is a | yellow-white F-type bright giant with an apparent magnit |
It is a | yellow-white F-type main sequence star with an apparent |
s Carinae is a | yellow-white F-type bright giant with an apparent magnit |
Its fainter companion is a | yellow-white F-type dwarf with an apparent magnitude of |
Nu Aquilae is a | yellow-white F-type supergiant with an apparent magnitud |
ω1 Aquarii is a | yellow-white F-type subgiant with an apparent magnitude |
ο2 Cancri is a | yellow-white F-type subgiant with an apparent magnitude |
Gamma Tucanae is a | yellow-white F-type giant with an apparent magnitude of |
panion, ξ2 Centauri B, is a tenth magnitude | yellow-white F-type dwarf. |
It is an eleventh magnitude, | yellow-white F-type main sequence dwarf. |
υ1 Cancri is a | yellow-white F-type giant with an apparent magnitude of |
1 Centauri is a | yellow-white F-type subgiant with an apparent magnitude |
Rho Telescopii is a | yellow-white F-type main sequence dwarf with an apparent |
Its companion, C Carinae B, is a | yellow-white F-type main sequence dwarf with an apparent |
The primary component, p Velorum A, is a | yellow-white F-type subgiant with an apparent magnitude |
The primary component, γ2 Caeli A, is a | yellow-white F-type giant with a mean apparent magnitude |
The primary component, b Velorum A, is a | yellow-white F-type supergiant with a mean apparent magn |
χ Cancri is a | yellow-white F-type main sequence dwarf with an apparent |
Its companion, γ¹ Volantis, is a | yellow-white F-type main sequence dwarf with an apparent |
component, Beta Trianguli Australis A, is a | yellow-white F-type giant with an apparent magnitude of |
Psi Tauri is a | yellow-white F-type main sequence dwarf with an apparent |
Mu Telescopii is a | yellow-white F-type main sequence dwarf with an apparent |
imary component, Epsilon Sculptoris A, is a | yellow-white F-type subgiant with an apparent magnitude |
β Caeli is a | yellow-white F-type main sequence dwarf with an apparent |
The brightest star, Kappa Tucanae A, is a | yellow-white F-type subgiant with an apparent magnitude |
49 Camelopardalis is a | yellow-white F-type main sequence dwarf with a mean appa |
primary component, 23 Ursae Majoris A, is a | yellow-white F-type subgiant with an apparent magnitude |
ν Caeli is a | yellow-white F-type main sequence dwarf with an apparent |
δ2 Canis Minoris is a | yellow-white F-type main sequence dwarf with an apparent |
ary component, Sigma² Ursae Majoris A, is a | yellow-white F-type subgiant with an apparent magnitude |
4 Canum Venaticorum is a | yellow-white F-type giant with a mean apparent magnitude |
The primary component, Psi Velorum A, is a | yellow-white F-type subgiant with an apparent magnitude |
The companion, Psi Velorum B, is a | yellow-white F-type main sequence dwarf, with an apparen |
π Canis Majoris A is a | yellow-white F-type subgiant with an apparent magnitude |
primary component, η Canis Minoris A, is a | yellow-white F-type giant with an apparent magnitude of |
Zeta Serpentis is a | yellow-white F-type main sequence dwarf with an apparent |
b² Carinae is a | yellow-white F-type main sequence dwarf with an apparent |
The brighter component is a | yellow-white F-type main sequence dwarf with an apparent |
imary component, Pi-2 Ursae Minoris A, is a | yellow-white F-type star with an apparent magnitude of + |
ξ2 Capricorni is a | yellow-white F-type main sequence dwarf with an apparent |
20 Canum Venaticorum is a | yellow-white F-type giant with a mean apparent magnitude |
Both components of the binary star are | yellow-white F-type stars and they have an orbital perio |
e is a spectroscopic binary composed of two | yellow-white F-type main sequence dwarfs with a combined |
ry component, Upsilon Ursae Majoris A, is a | yellow-white F-type subgiant with a mean apparent magnit |
The companion, 25 Canum Venaticorum B, is a | yellow-white F-type main sequence dwarf with an apparent |
blue-white B-type main sequence dwarf and a | yellow-white F-type main sequence dwarf. |
It is a | yellow-white F-type bright giant with an apparent magnit |
composed of two main sequence stars, one a | yellow-white F-type dwarf and the other a yellow G-type |
The primary component, ο Aquilae A, is a | yellow-white F-type main sequence dwarf with an apparent |
Its companion, ν1 Canis Majoris B is a | yellow-white F-type main sequence star with an apparent |
This is a | yellow-white F-type giant with an apparent magnitude of |
μ Capricorni is a | yellow-white F-type giant with an apparent magnitude of |
It is a | yellow-white F-type subgiant with an apparent magnitude |
It is a | yellow-white F-type main sequence dwarf with an apparent |
V509 Cassiopeiae is a | yellow-white G-type hypergiant with a mean apparent magn |
saw 2005 GC winner Bobby Julich retain the | yellow/white GC leader's jersey after defeating Kazakh A |
Sigma Columbae is a | yellow-white giant star in the constellation Columba. |
The star is classified as a | yellow-white giant (spectral class F2 III). |
Nu Persei is a highly luminous | yellow-white giant located about 555 light-years from Ea |
e immediately in air, with steel burning at | yellow-white heat. |
temperature range gives the F-type stars a | yellow-white hue. |
arent magnitude of +1.83, and is a white or | yellow-white in colour. |
seconds down on Bobby Julich) took over the | yellow/white jersey due to the time bonus awarded to sta |
It is a solitary, | yellow-white main sequence dwarf. |
Zeta Doradus is a solitary, | yellow-white, main sequence (F7 V) star located thirty-e |
HD 212301 is a | yellow-white main sequence star located approximately 17 |
HD 50554 is a | yellow-white main-sequence star [F8V] that currently fus |
Chalk-white, | yellow-white or grey. |
HD 15115 is a | yellow-white star. |
t is probably a large and powerful white to | yellow-white star. |
The component stars are nearly-identical | yellow-white stars in a tight orbit. |
It has a beautiful | yellow-white stripe that sweeps along its head, and red |
f its relatives, it has a striking white or | yellow-white stripe that extends down its thigh. |
Nu1 Columbae is a | yellow-white subgiant star in the constellation Columba. |
The star is classified as a | yellow-white supergiant (spectral class F8 Iab). |
A | yellow-white supergiant, it lies around 590 light years |
Larvae are mature at around 11mm, They are | yellow-white to salmon brown, with markings of black and |
Spectral type of the star is type F | yellow-white very metal rich dwarf star, slightly hotter |
e, consisting of generally small, black and | yellow/white wasp-like species. |
The male is mostly pale | yellow-white with a red crown and red bar across the bac |
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