「spectroscopic」の共起表現(2語左で並び替え)

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「spectroscopic」の共起表現一覧(2語左で並び替え)

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This is a single-lined	spectroscopic binary system.
VV Corvi (VV Crv) is a close	spectroscopic binary in the Corvus constellation.
Theta Cephei is a white	spectroscopic binary star, located about 135 light-years
Alpha Equulei is a unique	spectroscopic binary star consisting of two components.
A suspected	spectroscopic binary, it has now been resolved by speckl
It is a suspected	spectroscopic binary, although this has not been confirm
(ε Her, ε Herculis) is a fourth-magnitude	spectroscopic binary star in the constellation Hercules.
Nu Scorpii A is itself a semi-detached	spectroscopic binary, having a fainter B-type companion
omedae was discovered to be a double-lined	spectroscopic binary in a series of spectra taken in 189
Muterspaugh and M. Williamson at a robotic	spectroscopic telescope in Arizona, cf.).
imation of this coupling provides a direct	spectroscopic route to the distance between nuclei and h
SBC7 is an acronym for	Spectroscopic Binary 7th Catalogue.
of the pair, Kappa Pegasi B, is actually a	spectroscopic binary, with the components designated Kap
llipsometry (MOGE) is an advanced infrared	spectroscopic ellipsometry technique for studying free c
In all three	spectroscopic methods, the sample usually needs to be pr
harges was raised sufficiently to allow of	spectroscopic investigation.
olume of observations produced, along with	spectroscopic observations and some pioneering attempts
It is also a	spectroscopic binary star with a period of almost 273 da
It is also a	spectroscopic binary, and is composed of two stars with
Tau Puppis is also a	spectroscopic binary star system in which the multiple c
ful to confirm the result, although modern	spectroscopic techniques (e.g.
Sigma Aquilae is an eclipsing	spectroscopic binary.
, Epsilon Ursae Minoris A, is an eclipsing	spectroscopic binary.
31 Camelopardalis is an eclipsing	spectroscopic binary in the constellation Camelopardalis
ae (V415 Car or A Carinae) is an eclipsing	spectroscopic binary of the Algol type in the constellat
s (τ CMa, τ Canis Majoris) is an eclipsing	spectroscopic binary in the constellation Canis Major an
th other contractors to develop an Advance	Spectroscopic Portal (ASP) to allow border officials to
Biochemical and Mass	Spectroscopic analysis revealed that this pyroptosome is
Emission Pumping (SEP, or "PUMP and DUMP")	spectroscopic method.
Both visible and infrared	spectroscopic results indicate that Ixion's surface is a
ectrography for Rocky Exoplanet and Stable	Spectroscopic Observations, dubbed ESPRESSO, might allow
Nu Andromedae is	spectroscopic binary whose components are a blue-white B
due to the Doppler effect, they are called	spectroscopic binaries.
binary star, whose two components are both	spectroscopic binaries themselves, making a four-star sy
They are a	spectroscopic binary, meaning the separation between the
The star has also been identified as a	spectroscopic binary with a period of 494 days, but the
The system itself has been identified as a	spectroscopic binary star system; this means that Delta
metric, with a larger number available for	spectroscopic work and direct imaging photometry.
The star has been found to be a	spectroscopic binary star.
In 1898 this system was reported to be a	spectroscopic binary system, with an orbital period of 2
nt distance of 5".1 while it may also be a	spectroscopic binary.
This star is suspected of being a	spectroscopic binary, although this has not yet been con
e closest approach to this resolution by a	spectroscopic neutron instrument type, namely the backsc
Despite this, chemical and	spectroscopic testing indicates that the photograph is a
solution Transmission) is a compilation of	spectroscopic parameters that a variety of computer code
Beta Cephei is a triple star comprising a	spectroscopic binary with a magnitude 8 optical companio
und was characterized by computational and	spectroscopic techniques and found to possess a cage-lik
ed to phycobiliproteins to confer specific	spectroscopic properties.
freely accessible, and contains extensive	spectroscopic data for organic compounds including that
second per century, which corresponds from	spectroscopic observations to 20-30 km−1).
infrared, but does not cover time-resolved	spectroscopic techniques.
uting is an approach to the development of	spectroscopic instruments, particularly for industrial a
ibutions to science are the development of	spectroscopic tools and their applications, in particula
ve a companion, which would make Electra a	spectroscopic binary.
became the Reuven Ramaty High Energy Solar	Spectroscopic Imager (RHESSI), the first space mission n
The Reuven Ramaty High Energy Solar	Spectroscopic Imager (RHESSI), Explorer 81, images solar
The Far Ultraviolet	Spectroscopic Explorer (FUSE) is a space-based telescope
First discovered	spectroscopic binary in 1889 by an American astronomer E
67 jointly with William Huggins, for their	spectroscopic study of the composition of stars.
of the system components, A and B, form a	spectroscopic binary that completes an orbit every 76 ye
esolved with optical telescopes, forming a	spectroscopic binary.
A is separated from its	spectroscopic companion by 0.05 arcseconds.
erally obtained empirically from gas-phase	spectroscopic studies of atoms.
uctases depending on their function, their	spectroscopic properties, and their catalytic properties
He identified this gas by	spectroscopic methods to be nitrogen.
This instrument had a	spectroscopic range of 82.5 to 185 nms, and a spectral r
at showed radio loud quasars have distinct	spectroscopic signatures that depend on their orientatio
nstruments, incorporating both imaging and	spectroscopic data at optical, infrared, and radio wavel
Gamma rays detected in a	spectroscopic system produce peaks in the spectrum.
Donati was also a pioneer in the	spectroscopic study of the stars and the sun.
He became interested in using	spectroscopic methods including nuclear magnetic resonan
of predictive models for use in real-time	spectroscopic analysis of materials.
us Doppler shift analysis included face-on	spectroscopic binaries.
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
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.
Zeta Trianguli Australis (ζ TrA) is a	spectroscopic binary in the constellation Triangulum Aus
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.
It is a	spectroscopic binary, whose components are separated by
It is a	spectroscopic binary with a faint class-G companion.
17 Leporis (17 Lep) is a	spectroscopic binary star in the constellation of Lepus.
ilon Sagittarii (υ Sgr, υ Sagittarii) is a	spectroscopic binary star system in the constellation Sa
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
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 star is a	spectroscopic binary, and the primary is also a Beta Cep
is its very high basicity; another is its	spectroscopic properties.
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
It is a	spectroscopic binary, and the two subcomponents have app
Chi Aurigae is a	spectroscopic binary which is classified as a blue-white
It is a	spectroscopic binary, which means it is a binary star wi
name HR 2422 Monocerotis or HR 2422) is a	spectroscopic binary at a distance of around 6600 light-
Atik is a	spectroscopic binary star consisting of a spectral type
It is a	spectroscopic binary having a 113.8 day period, indicati
Kappa Arietis is a	spectroscopic binary which is classified as a white A-ty
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 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
is not possible to isolate or detect it by	spectroscopic means
aries detected in this manner are known as	spectroscopic binaries.
effects of weak gravitational lensing) and	Spectroscopic All Sky Cosmic Explorer (SPACE, to measure
target-of-opportunity basis, less frequent	spectroscopic measurements complement the rapid photomet
y Notices Roy Astron Soc, vol lxv, 1905); '	Spectroscopic Observations of the Great Sunspot (Februar
Also called 1H-nuclear magnetic resonance	spectroscopic imaging and proton magnetic resonance spec
Magnetic resonance	spectroscopic imaging is a noninvasive imaging method th
ject was known as Small Main-belt Asteroid	Spectroscopic Survey, Phase II or SMASSII, which built o
a permanent dipole moment, which makes the	spectroscopic characterization easier.
ve diseases and the use of microscopic and	spectroscopic methods in neurosciences (“neurophotonics”
mmonly used in fluorescence microscopy and	spectroscopic applications for selection of the excitati
FM can be operated in the imaging mode and	spectroscopic mode.
ng the structure of atoms and molecules by	spectroscopic methods.
ion to the new equilibrium is monitored by	spectroscopic probes such as fluorescence or less freque
However, more detailed	spectroscopic observations in 2005 appear to show that i
rs prefer the name TPD because it is not a	spectroscopic method.
ber Rydberg states has spawned a number of	spectroscopic techniques.
rferometer was used to resolve a number of	spectroscopic binary systems, including Alpha Andromedae
It consists of a	spectroscopic binary and a third component.
de determination the orbital period of A's	spectroscopic binary difficult.
ei is a triple star system consisting of a	spectroscopic double star with a wider companion.
An advantage of this	spectroscopic technique is that the ions can be detected
The system consists of a	spectroscopic binary with a yellow G-type supergiant and
The orbit of a	spectroscopic binary is determined by making a long seri
his work in development of ultrasensitive	spectroscopic methods with applications in trace gas det
vae, he has also worked extensively on the	spectroscopic studies of Active Galactic Nuclei
As an optical technique,	spectroscopic ellipsometry is non-destructive and contac
nings are the Photometric parallax method,	Spectroscopic parallax, and Dynamical parallax
s contributions to Astronomical Physics by	spectroscopic observations of eclipses, solar pre-eminen
purity and served as reliable reagents and	spectroscopic standards.
provide high resolution, multi-wavelength	spectroscopic observations.
larization spectroscopy comprises a set of	spectroscopic techniques based on polarization propertie
ited to spectroscopy, although some useful	spectroscopic work can be performed with reflecting type
trophysics (ASCA) for a spatially resolved	spectroscopic analysis of Abell 2256 over the energy ban
to prove the existence of this species by	spectroscopic means
Both bright stars are	spectroscopic binaries and have at least one closer comp
ures of variable stars, cluster stars, and	spectroscopic binaries; and astrometry of minor planets
RI scanner for functional, structural, and	spectroscopic studies of humans and animals.
The presence of water ice is supported by	spectroscopic observations, which have revealed crystall
Xi Tauri a	spectroscopic and eclipsing triple star.
Carl Vogel, Pickering discovered the first	spectroscopic binary stars.
ame logic follows to explain the identical	spectroscopic results provided by the hydrogen atoms on
boratory, in which he assembled the latest	spectroscopic equipment.
resolved Pismis 24-1SW and the unresolved	spectroscopic binary Pismis 24-1NE.
Their individual	spectroscopic classifications are dK5e and dK7e.
adial velocity most commonly refers to the	spectroscopic radial velocity.
FOS was designed to make	spectroscopic observations of astrophysical sources from
UT) was a space telescope designed to make	spectroscopic observations in the far-ultraviolet region
-class stars, are themselves thought to be	spectroscopic binaries, bringing the total number of sta
The Hubble Space Telescope took STIS/UV	spectroscopic observations on May 3, 2010.
P Cygni gives its name to a type of	spectroscopic feature called a P Cygni profile, where th
using a	spectroscopic technique, such as infrared spectroscopy,
Kappa Velorum is	spectroscopic binary which is classified as a blue-white
With this	spectroscopic evidence a search for these type of molecu
the subject of numerous X-ray diffraction,	spectroscopic and theoretical studies.

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「spectroscopic」の共起表現一覧(2語左で並び替え)