「SPECTROSCOPIC」の共起表現(1語左が「a」)

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共起表現

「SPECTROSCOPIC」の共起表現一覧(1語左が「a」)

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Component A is a	spectroscopic binary.
HD 37017 is a	spectroscopic binary.
Lambda Virginis is a	spectroscopic binary.
IU Aurigae is a	spectroscopic binary.
EZ Aquarii AC is a	spectroscopic binary.
rimary component, Epsilon Volantis A, is a	spectroscopic binary.
3 Camelopardalis is a	spectroscopic binary in the constellation Camelopardalis
Xi Tauri a	spectroscopic and eclipsing triple star.
It consists of a	spectroscopic binary and a third component.
12 Camelopardalis is a	spectroscopic binary in the constellation Camelopardalis
V373 Cas is a	spectroscopic binary in the constellation Cassiopeia.
V357 Carinae (a Car, a Carinae) is a	spectroscopic binary in the constellation Carina.
Theta-1 Sagittarii is a	spectroscopic binary lying 617 light years from Earth.
θ1 Crucis (θ1 Cru, Theta1 Crucis) is a	spectroscopic binary star in the constellation Crux.
The star e Serpentis (e Ser) is a	spectroscopic binary in the constellation of Serpens.
It is a	spectroscopic binary whose components have an orbital pe
It is a	spectroscopic binary whose components have an orbital pe
It is a	spectroscopic binary with an orbital period of 143.6065
Pi Andromedae (π And, π Andromedae) is a	spectroscopic binary in the constellation Andromeda.
It is a	spectroscopic binary and has a companion located 0.12 ar
Secondary, Σ 1694 B is a	spectroscopic binary both A-type main sequence star.
It is a	spectroscopic binary whose two components are separated
104 Aqr A is a	spectroscopic binary and is suspected to be variable.
Lambda Andromedae is a	spectroscopic binary with an orbital period of 20.52 day
It is a	spectroscopic binary with an orbital period of 134 days.
θ2 Crucis (θ2 Cru / Theta2 Crucis) is a	spectroscopic binary star in the constellation Crux.
This star is suspected of being a	spectroscopic binary, although this has not yet been con
Zeta Trianguli Australis (ζ TrA) is a	spectroscopic binary in the constellation Triangulum Aus
Gamma rays detected in a	spectroscopic system produce peaks in the spectrum.
It is a	spectroscopic binary whose components have magnitudes of
Pi4 Orionis (π4 Ori, π4 Orionis) is a	spectroscopic binary star in the constellation Orion.
The star has been found to be a	spectroscopic binary star.
It is a	spectroscopic binary, whose components are separated by
It is a	spectroscopic binary with a faint class-G companion.
rs prefer the name TPD because it is not a	spectroscopic method.
17 Leporis (17 Lep) is a	spectroscopic binary star in the constellation of Lepus.
Beta Cephei is a triple star comprising a	spectroscopic binary with a magnitude 8 optical companio
ilon Sagittarii (υ Sgr, υ Sagittarii) is a	spectroscopic binary star system in the constellation Sa
using a	spectroscopic technique, such as infrared spectroscopy,
The primary is a	spectroscopic binary, and its close companion completes
Theta Aquilae is a	spectroscopic binary classified as a blue-white B-type g
omponent, Iota Trianguli Australis A, is a	spectroscopic binary with a mean apparent magnitude of +
Iota Arietis is a	spectroscopic binary classified as a yellow G-type super
of the system components, A and B, form a	spectroscopic binary that completes an orbit every 76 ye
ei is a triple star system consisting of a	spectroscopic double star with a wider companion.
It is a	spectroscopic binary with components that are too close
anis Majoris (ζ CMa, ζ Canis Majoris) is a	spectroscopic binary in the constellation Canis Major.
Gliese 678 is a	spectroscopic binary star system approximately 60 light-
This is a	spectroscopic binary, which means that the individual co
HD 176051 is a	spectroscopic binary star system located approximately 4
This instrument had a	spectroscopic range of 82.5 to 185 nms, and a spectral r
It is also a	spectroscopic binary star with a period of almost 273 da
This star is a	spectroscopic binary, and the primary is also a Beta Cep
In 1898 this system was reported to be a	spectroscopic binary system, with an orbital period of 2
omedae (Eta And, η Andromedae, η And) is a	spectroscopic binary star in the constellation of Androm
Linear dichroism (LD) is a	spectroscopic technique that is primarily used to study
Rho Tucanae is a	spectroscopic binary composed of two yellow-white F-type
nt distance of 5".1 while it may also be a	spectroscopic binary.
They are a	spectroscopic binary, meaning the separation between the
e closest approach to this resolution by a	spectroscopic neutron instrument type, namely the backsc
It is a	spectroscopic binary, and the two subcomponents have app
Chi Aurigae is a	spectroscopic binary which is classified as a blue-white
The system consists of a	spectroscopic binary with a yellow G-type supergiant and
It is a	spectroscopic binary, which means it is a binary star wi
esolved with optical telescopes, forming a	spectroscopic binary.
name HR 2422 Monocerotis or HR 2422) is a	spectroscopic binary at a distance of around 6600 light-
of the pair, Kappa Pegasi B, is actually a	spectroscopic binary, with the components designated Kap
The star has also been identified as a	spectroscopic binary with a period of 494 days, but the
Atik is a	spectroscopic binary star consisting of a spectral type
It is a	spectroscopic binary having a 113.8 day period, indicati
The orbit of a	spectroscopic binary is determined by making a long seri
Kappa Arietis is a	spectroscopic binary which is classified as a white A-ty
ve a companion, which would make Electra a	spectroscopic binary.
Reflectance difference spectroscopy is a	spectroscopic technique which measures the difference in
l magnitude of approximately 5.15 and is a	spectroscopic binary star which consists of two giant st
The system itself has been identified as a	spectroscopic binary star system; this means that Delta
It is also a	spectroscopic binary, and is composed of two stars with
The Rossiter-McLaughlin effect is a	spectroscopic phenomenon observed when either an eclipsi
At the centre of the system is a	spectroscopic binary, Iota Serpentis A and B. These are
Tau Puppis is also a	spectroscopic binary star system in which the multiple c

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「SPECTROSCOPIC」の共起表現一覧(1語左が「a」)