例文 | 共起表現 |
「ζ」の共起表現一覧(1語右で並び替え)
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The factors Q, damping ratio | ζ, and attenuation α are related such that |
has the α, β and ε, Vela has γ and δ, Puppis has | ζ, and so on. |
Zeta Apodis ( | ζ Aps, ζ Apodis) is a star in the constellation Ap |
Zeta Arae ( | ζ Ara, ζ Arae) is a star in the constellation Ara. |
ociation consisting this star, along with ε Ari, | ζ Ari, π Ari, and ρ3 Ari |
It seems unlikely that | ζ as used here can meaningfully be regarded as an |
Finally, the stars α Aur, ε Aur, | ζ Aur, and η Aur form the charioteer's nose: η Aur |
It is composed of the stars | ζ Aurigae Hoedus I and η Aurigae Hoedus II, where |
The deviation | ζ between the ellipsodidal height h and the normal |
The components of ζ² Cancri are denoted | ζ Cancri C and ζ Cancri D. ζ Cancri C is the brigh |
The tenth magnitude | ζ Cancri D has the color of a red dwarf, and may i |
ζ Canis Majoris is approximately 336 light years f | |
It has an unseen companion, | ζ Canis Majoris B. The two stars orbit around thei |
The primary component, | ζ Canis Majoris A, is a blue-white B-type main seq |
Zeta Capricorni, ( | ζ Cap, ζ Capricorni), is a fourth-magnitude star i |
Its companion, | ζ Capricorni B is a white dwarf. |
ζ Capricorni is a binary star, with the primary co | |
The | ζ Capricorni binary system is approximately 398 li |
ζ Cas is a member of an unusual group of variable | |
Zeta Cassiopeiae ( | ζ Cas, ζ Cassiopeiae) is a star in the constellati |
ζ Cassiopeiae is a blue-white B-type subgiant with | |
Zeta Canis Majoris ( | ζ CMa, ζ Canis Majoris) is a spectroscopic binary |
Zeta Cancri ( | ζ Cnc, ζ Cancri) is a star system in the constella |
ζ Crucis (ζ Cru, Zeta Crucis) is a binary star in | |
ζ Crucis is located at about 360 light-years from | |
Zeta Cygni ( | ζ Cyg) and CCDM J21129+3014B form a binary star sy |
Here | ζ denotes the Riemann zeta function and π the prim |
ine of charging hyenas (ι Dra, θ Dra, η Dra, and | ζ Dra). |
Zeta Draconis ( | ζ Dra, ζ Draconis) is a star in the constellation |
e Phoenician letter gave rise to the Greek Zeta ( | Ζ), Etruscan z , Latin Z, and Cyrillic Ze З. |
It use letter | Ζ for επτα (seven). |
The use of the Greek letter zeta ( | ζ) for a function previously mentioned by Euler |
Zeta Geminorum ( | ζ Gem, ζ Geminorum) is a star in the constellation |
β, -γ and -δ genes are intronless and C/EBPε and | -ζ have respectively two and four exons that lead i |
Zeta Herculis ( | ζ Her, ζ Herculis) is a binary star system in the |
Besides | ζ Herculis, the group includes δ Trianguli, ζ Reti |
I, ε Hya as Minazal III, ρ Hya as Minazal IV and | ζ Hya as Minazal V (exclude σ Hya) |
I, ε Hya as Minazal III, ρ Hya as Minazal IV and | ζ Hya as Minazal V (exclude σ Hya) |
This star, along with δ Hya (Lisan al Sudja), | ζ Hya, η Hya, ρ Hya and σ Hya (Minhar al Shija), w |
ter including this star, δ Hya (Lisan al Sudja), | ζ Hya, η Hya, ρ Hya and σ Hya (Minhar al Shija). |
This star, along with ε Hya, | ζ Hya, η Hya, ρ Hya and σ Hya (Minhar al Shija), w |
ζ is electrokinetic potential | |
where | ζ is the Riemann zeta function. |
The 12 images of the line though the point (1: | ζ: ζ2: ζ3: ζ4) and its complex conjugate, where ζ |
c viscosity of the dispersion medium (Pa s), and | ζ is zeta potential (i.e., the electrokinetic pote |
Zeta Leonis ( | ζ Leo, ζ Leonis) is a fourth-magnitude star in the |
evaluated on a simple (decomposable) (2ν)-vector | ζ of unit volume, is bounded above by . |
Zeta Ophiuchi ( | ζ Oph, ζ Ophiuchi) is a star located in the conste |
In April 2010, the naked-eye star | ζ Ophiuchi was occulted by 824 Anastasia. |
Although | ζ Ophiuchi is a hot blue supergiant star it appear |
Discoveries announced in early 2011 show that | ζ Ophiuchi is moving through space at 87,000 km/h |
ζ Ophiuchi is roughly half way through the initial | |
Association along with the "Orion's Belt" stars | ζ Ori (Alnitak), ε Ori (Alnilam), and δ Ori (Minta |
Zeta Phoenicis ( | ζ Phe, ζ Phoenicis) is a 280 light-year distant st |
The MSZ-006A1B | Ζ Plus was designed to operate mainly in its waver |
The A1B | Ζ Plus functioned as an atmospheric fightercraft, |
better flight within Earth's atmosphere the A1B | Ζ Plus had longer, more sweeping, wings to provide |
The A1B | Ζ Plus could carry an assortment of guided missile |
rmed whether Amuro Ray actually test-piloted the | Ζ Plus A1, and the rumor may have just been a mark |
oup includes besides Zeta Herculis: δ Trianguli, | ζ Reticuli, 1 Hydrae, Gl 456, Gl 678, and Gl 9079. |
This group includes: δ Trianguli, φ2 Pavonis, | ζ Reticuli, 1 Hydrae, Gl 456, Gl 678, and Gl 9079. |
easily found on the sky, being close to the star | ζ Sagittarii. |
ζ Sco; applied to Becvar's star list, as Grafias. | |
Zeta Serpentis ( | ζ Ser, ζ Serpentis) is a star in the constellation |
Zeta Sagittarii ( | ζ Sgr, ζ Sagittarii) is the third brightest star s |
Zeta Telescopii ( | ζ Tel, ζ Telescopii) is the second brightest star |
Zeta Trianguli Australis ( | ζ TrA) is a spectroscopic binary in the constellat |
n alternative name of Mizar, Zeta Ursae Majoris ( | ζ UMa). |
Zeta Ursae Minoris ( | ζ UMi, ζ Ursae Minoris) is a star in the constella |
例文 | 共起表現 |
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