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Weblio 辞書 > 英和辞典・和英辞典 > ζに関連した共起表現

「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
                                                                                                   


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