「apparent.」の共起表現(1語右で並び替え)6ページ目

「apparent.」の共起表現一覧(1語右で並び替え)6ページ目

apparent.

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e is a blue-white B-type subgiant with a mean apparent magnitude of +4.66.
Its apparent magnitude is 6.14.
Bayer gave Thuban the designation Alpha, its apparent magnitude of 3.65 is 3.7 times fainter than t
Papagena comes to a favorable near-opposition apparent magnitude of better than magnitude 9.8 every
Catalog 2000) and features a yellow giant of apparent magnitude +7.9 and spectral type G0 as its br
Its apparent magnitude is 5.89.
k Carinae is a yellow G-type giant with an apparent magnitude of +4.79.
blue-white B-type main sequence dwarf with an apparent magnitude of +4.97.
white A-type main sequence dwarf which has an apparent magnitude of +9.5v and is separated from the
Its apparent magnitude is 5.68.
orpii is a yellow G-type bright giant with an apparent magnitude of +4.31.
ively belongs to spectral class G0III and has apparent magnitude +3.92 and a luminosity approximatel
Its apparent magnitude is 5.44.
ψ Centauri is a white A-type subgiant with an apparent magnitude of +4.05.
Scorpii is a blue-white B-type dwarf with an apparent magnitude of +3.93.
sage it is only expected to brighten to about apparent magnitude 17.
icorni is a yellow-white F-type giant with an apparent magnitude of +5.08 and is approximately 90.2
Its apparent magnitude is 5.30.
Both are open clusters and being 7th apparent magnitude objects they are easy targets with
rni A, sometimes called ο¹ Capricorni, has an apparent magnitude of +5.94, while the companion, ο Ca
-white B-type main sequence dwarf with a mean apparent magnitude of +5.22.
white A-type main sequence dwarf with a mean apparent magnitude of +4.64.
fied as an irregular variable and experiences apparent magnitude fluctuations between +4.51 and +4.6
08 B. The fourth component, HD 72108 C has an apparent magnitude of +9.3, and is 19 arcseconds from
Its apparent magnitude is 6.37.
orpii is a blue-white B-type subgiant with an apparent magnitude of +3.56.
panion is a yellow-white F-type dwarf with an apparent magnitude of +7.72.
blue-white B-type main sequence dwarf with an apparent magnitude of +5.26.
Its apparent magnitude is 5.60.
The binary has an apparent magnitude of +4.53 and an orbital period of 4
It is an orange K-type giant with an apparent magnitude of +4.23, and is approximately 158
Its apparent magnitude is 5.20.
Rho2 Arietis is a M-type red giant with an apparent magnitude which varies between 5.62 and 6.01.
is a white A-type main sequence dwarf with an apparent magnitude of +2.7.
Normally, the combined apparent magnitude varies between 14.0 and 15.1; durin
Its apparent magnitude is 4.53.
s faint companion (CCDM J05396-3404 B) has an apparent magnitude of 12.3m and is 13.5" distant from
s a yellow G-type main sequence dwarf with an apparent magnitude of +7.2.
Its apparent magnitude is 6.04.
lorum is a blue-white B-type subgiant with an apparent magnitude of +4.85.
classified as an orange K-type giant, with an apparent magnitude of +6.44.
llow-white F-type main sequence dwarf with an apparent magnitude of +5.17.
57 Cancri B is an orange K-type star with an apparent magnitude of +6.6.
Its apparent magnitude is 5.19.
lta Arietis is an orange K-type giant with an apparent magnitude of +4.35.
ttarii is a spectral type K0 giant and has an apparent magnitude of +4.12.
57 Cancri A, is a yellow G-type giant with an apparent magnitude of +6.1.
It is an orange K-type giant with an apparent magnitude of +4.66 and is approximately 188.4
Its apparent magnitude is 6.87.
a blue O-type main sequence dwarf with a mean apparent magnitude of +5.99.
blue-white B-type main sequence dwarf with an apparent magnitude of +4.81 and is approximately 542 l
scovery of 76,000 galaxies brighter than 18th apparent magnitude in a third of the southern sky, bas
st's detection revealed a blue galaxy with an apparent magnitude of 24.95 ± 0.11.
Its apparent magnitude is +6.45.
Telescopii is an orange K-type giant with an apparent magnitude of +4.88.
llow-white F-type main sequence dwarf with an apparent magnitude of +5.12.
Its apparent magnitude is 5.0
It has apparent magnitude 6.47 and is about 200 light-years a
llow-white F-type main sequence dwarf with an apparent magnitude of +7.9.
heid variable star and as such has a variable apparent magnitude of +3.7 to +4.2, with period of app
Its apparent magnitude is 5.52.
orni is an orange K-type bright giant with an apparent magnitude of +5.28.
is a white A-type main sequence dwarf with an apparent magnitude of +5.3.
Its apparent magnitude is 5.93.
Kappa Leonis has apparent magnitude +4.46 and has a stellar classificat
Ras Alhague has an apparent magnitude of +2.08, belongs to the spectral c
Its apparent magnitude is 6.55.
ellow-white F-type main sequence star with an apparent magnitude of +4.48.
a² Antliae is a white A-type subgiant with an apparent magnitude of +5.91.
-white B-type main sequence dwarf with a mean apparent magnitude of +4.36.
Its apparent magnitude is 5.07.
27P/Crommelin was recovered on 12 May 2011 at apparent magnitude 18.7.
is a white A-type main sequence dwarf with an apparent magnitude of +4.72.
is δ² Apodis, an orange K-type giant with an apparent magnitude of +5.27.
Its apparent magnitude is 4.64.
Epsilon Corvi has apparent magnitude +3.02 and belongs to the spectral c
δ¹ Apodis, is a M-type red giant with a mean apparent magnitude of +4.68.
Its apparent magnitude is 5.10.
Sculptoris is an orange K-type giant with an apparent magnitude of +5.30.
mma Ceti belongs to spectral class A2 and has apparent magnitude +2.7.
s is a blue-white B-type subgiant with a mean apparent magnitude of +3.50.
sky, is a spectral type F2 giant which has an apparent magnitude of +4.27.
identical to SN 1054, it would shine with an apparent magnitude of -8.71, about 1/40 as bright as t
Its apparent magnitude is 5.48.
It has an apparent magnitude of 11.33 and an absolute magnitude
At an apparent magnitude of +4.78 it is visible to the naked
Its apparent magnitude is 6.40.
The main star possesses an apparent magnitude of +1.5 and belongs to the spectral
Its apparent magnitude is 4.79.
yrae belongs to spectral class B2.5IV and has apparent magnitude of +4.39.
blue-white B-type main sequence dwarf with an apparent magnitude of +3.18.
Atlas A, is a blue-white B-type giant with an apparent magnitude of +3.62.
Its apparent magnitude is 5.71.
It is an orange K-type giant with an apparent magnitude of +3.12.
Its apparent magnitude is 4.54.
is a spectral type B2.5 subgiant which has an apparent magnitude of +4.37.
Its apparent magnitude is 6.10.
Nu Tucanae is a M-type red giant with a mean apparent magnitude of +4.91.
Pegasi is of spectral class G2II-III and has apparent magnitude +3.1.
passed perihelion on March 18, 2002, and with apparent magnitude 3.5, it became the brightest comet
The companion star, γ2 Caeli B, has an apparent magnitude of +9.6 and is located 0.886 arcsec
Its apparent magnitude is 6.33.
R Carinae is a M-type red giant with a mean apparent magnitude of +7.43.
ω Cancri is a yellow G-type giant with an apparent magnitude of +5.87.
s is a blue-white B-type bright giant with an apparent magnitude of +4.11.
Its apparent magnitude is 5.45.
is is an orange K-type supergiant with a mean apparent magnitude of +3.89.
a Telescopii is a yellow G-type giant with an apparent magnitude of +4.10.
white A-type main sequence dwarf with a mean apparent magnitude of +4.88.
ellow-white F-type main sequence star with an apparent magnitude of +7.65.
The apparent magnitude is 7.06.
onent is a yellow G-type bright giant with an apparent magnitude of +4.22.
is a white A-type main sequence dwarf with an apparent magnitude of +5.1.
blue-white B-type main sequence dwarf with an apparent magnitude of +4.27.
It has an apparent magnitude of 4.32m.
inae is a white A-type supergiant with a mean apparent magnitude of +4.59.
A, is a yellow-white F-type subgiant with an apparent magnitude of +4.5.
, is a blue-white B-type subgiant with a mean apparent magnitude of +5.13.
rae is a blue-white B-type supergiant with an apparent magnitude of +3.65.
Its apparent magnitude may have reached as high as -7, lea
It has an apparent magnitude of 4.69m.
It is a blue-white B-type giant with an apparent magnitude of +3.96 and is approximately 499 l
Capricorni is an orange K-type giant with an apparent magnitude of +6.76.
Majoris A, is a white A-type subgiant with an apparent magnitude of +3.12.
Maximum apparent magnitude was approximately +8.
Carinae is a blue-white B-type giant with an apparent magnitude of +3.29.
e F-type main sequence dwarfs with a combined apparent magnitude of +5.38.
binary, consisting of two stars each with an apparent magnitude of +6.4.
HD 75063 is a white A-type giant with an apparent magnitude of +3.87.
ron Virginis is a yellow G-type giant with an apparent magnitude of +4.12.
ctral type A3 main sequence star which has an apparent magnitude of +4.54.
illion Kilometer) and will be as bright as an apparent magnitude of 8.8.
It has an apparent magnitude of 4.06m.
ial Sun-like star (G5 spectral class) with an apparent magnitude of 7.3.
Its companion, η Capricorni B, has an apparent magnitude of +6.5 and is located 0.34 arcseco
It is a yellow-white F-type subgiant with an apparent magnitude of +3.99 and is approximately 52.9
s a yellow G-type main sequence dwarf with an apparent magnitude of +6.6.
is a white A-type main sequence dwarf with an apparent magnitude of +4.82.
blue-white B-type main sequence dwarf with an apparent magnitude of +4.82 and is approximately 400 l
sae Majoris is an orange K-type giant with an apparent magnitude of +5.15.
assified as a blue-white B-type giant with an apparent magnitude of +3.24.
Acubens is a fourth-magnitude star with an apparent magnitude of 4.20, making it barely visible t
n it came within 0.35 AU of the Earth with an apparent magnitude of 6.5.
It has an apparent magnitude of 4.14m.
At an apparent magnitude of 12.0, NGC 3982 needs a telescope
It has a combined apparent magnitude of +4.93 and is approximately 621 l
8 kiloparsecs) from the Earth with a very dim apparent magnitude of 25.
orange dwarf star (K7 spectral class) with an apparent magnitude of 8.9.
blue-white B-type main sequence dwarf with an apparent magnitude of +4.34.
r (G1V) in the constellation Aquarius with an apparent magnitude is 6.21.
blue main sequence primary of class B2 and an apparent magnitude of 4.01 and a hot subdwarf secondar
The brighter star, HD 222502, has an apparent magnitude of 7.73.
θ¹ has an apparent magnitude of +4.62 while the slightly dimmer
2010 apparition the comet became as bright as apparent magnitude 11.5.
white A-type main sequence dwarf with a mean apparent magnitude of +5.34.
The total nebula shines at the apparent magnitude of +10.1 with its central star or p
ncri C is the brighter of the pair, having an apparent magnitude of +6.12.
It has the apparent magnitude of 6.45.
Pi Persei has an apparent magnitude of +4.7 and spectral class A2V.
white B-type main sequence dwarf star with an apparent magnitude of +4.49.
ucanae is a white A-type subgiant with a mean apparent magnitude of +6.11.
Its apparent magnitude is 5.40 and its absolute magnitude
is a yellow-white F-type subgiant with a mean apparent magnitude of +3.78.
HD 78004 is an orange K-type giant with an apparent magnitude of +3.75.
00h 48m 57.7597s +22° 50′ 39.669″, having an apparent magnitude of 9.56
blue-white B-type main sequence dwarf with an apparent magnitude of +3.02.
Their combined apparent magnitude is +3.53.
ified a blue-white B-type subgiant and has an apparent magnitude of +4.35.
o Ursae Majoris is a M-type red giant with an apparent magnitude of +4.74.
A, is a yellow-white F-type subgiant with an apparent magnitude of +4.85.
iuchi belongs to spectral class A1V+A and has apparent magnitude +3.82.
alis A, is a spectroscopic binary with a mean apparent magnitude of +5.28.
an orange K-type main sequence dwarf with an apparent magnitude of +8.16.
t is a blue-white B-type bright giant with an apparent magnitude of +3.84 and is approximately 312 l
is a white A-type main sequence dwarf with an apparent magnitude of +4.56.
in an asterism, however, is not based on the apparent magnitude of this star as the Bayer system us
isam belongs to the spectral class K0 and has apparent magnitude +3.8.
Zeta Draconis is a giant star with an apparent magnitude of +3.17 and a spectral class of B9
ri A, is a blue-white B-type subgiant with an apparent magnitude of +3.13.
llow-white F-type main sequence dwarf with an apparent magnitude of +6.91.
10 Virginis is an orange K-type giant with an apparent magnitude of +4.39.
υ Capricorni is a M-type red giant with an apparent magnitude of +5.15.
ga Serpentis is a yellow G-type giant with an apparent magnitude of +5.21.
vation of a comet, though it never rose above apparent magnitude 3-4.
Its mean apparent magnitude is +4.52.
Carinae is an orange K-type giant with a mean apparent magnitude of +5.60.
i belongs to the spectral class A0 and has an apparent magnitude of +3.8.
rateris belongs to the spectral class K1, has apparent magnitude 4.07, and is 174 light years from E
It is a yellow G-type giant with an apparent magnitude of +5.01.
A, is a yellow-white F-type giant with a mean apparent magnitude of +6.32.
alis A, is an orange K-type sub-giant with an apparent magnitude of +4.11V.
is a white A-type main sequence dwarf with an apparent magnitude of +5.04 and is approximately 504 l
Though it has an apparent magnitude of only 4.914, its absolute visual
sae Majoris is an orange K-type giant with an apparent magnitude of +3.69.
e is a yellow-white F-type supergiant with an apparent magnitude of +4.64.
oris is a blue-white B-type giant with a mean apparent magnitude of +5.23.
dividual stars, of which the brightest are of apparent magnitude 13.1.
It is an orange K-type giant with an apparent magnitude of +3.78 and is approximately 96.8
white A-type main sequence dwarf with a mean apparent magnitude of +4.95.
It ranges in apparent magnitude from 1.59 to 1.64.

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