「SPECTROSCOPIC」の共起表現(2語右で並び替え)

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共起表現

「SPECTROSCOPIC」の共起表現一覧(2語右で並び替え)

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With this	spectroscopic evidence a search for these type of molecu
This star is suspected of being a	spectroscopic binary, although this has not yet been con
It is a suspected	spectroscopic binary, although this has not been confirm
Also called 1H-nuclear magnetic resonance	spectroscopic imaging and proton magnetic resonance spec
It consists of a	spectroscopic binary and a third component.
It is a	spectroscopic binary and has a companion located 0.12 ar
104 Aqr A is a	spectroscopic binary and is suspected to be variable.
Both bright stars are	spectroscopic binaries and have at least one closer comp
The primary is a	spectroscopic binary, and its close companion completes
This star is a	spectroscopic binary, and the primary is also a Beta Cep
metric, with a larger number available for	spectroscopic work and direct imaging photometry.
nings are the Photometric parallax method,	Spectroscopic parallax, and Dynamical parallax
It is a	spectroscopic binary, and the two subcomponents have app
uctases depending on their function, their	spectroscopic properties, and their catalytic properties
ibutions to science are the development of	spectroscopic tools and their applications, in particula
olume of observations produced, along with	spectroscopic observations and some pioneering attempts
und was characterized by computational and	spectroscopic techniques and found to possess a cage-lik
ures of variable stars, cluster stars, and	spectroscopic binaries; and astrometry of minor planets
It is also a	spectroscopic binary, and is composed of two stars with
Their individual	spectroscopic classifications are dK5e and dK7e.
Although	spectroscopic measurements are necessary to obtain a hig
name HR 2422 Monocerotis or HR 2422) is a	spectroscopic binary at a distance of around 6600 light-
nstruments, incorporating both imaging and	spectroscopic data at optical, infrared, and radio wavel
larization spectroscopy comprises a set of	spectroscopic techniques based on polarization propertie
Secondary, Σ 1694 B is a	spectroscopic binary both A-type main sequence star.
-class stars, are themselves thought to be	spectroscopic binaries, bringing the total number of sta
A is separated from its	spectroscopic companion by 0.05 arcseconds.
P Cygni gives its name to a type of	spectroscopic feature called a P Cygni profile, where th
ited to spectroscopy, although some useful	spectroscopic work can be performed with reflecting type
	Spectroscopic observations can be used in a myriad of co
Theta Aquilae is a	spectroscopic binary classified as a blue-white B-type g
Iota Arietis is a	spectroscopic binary classified as a yellow G-type super
target-of-opportunity basis, less frequent	spectroscopic measurements complement the rapid photomet
Rho Tucanae is a	spectroscopic binary composed of two yellow-white F-type
de determination the orbital period of A's	spectroscopic binary difficult.
ectrography for Rocky Exoplanet and Stable	Spectroscopic Observations, dubbed ESPRESSO, might allow
a permanent dipole moment, which makes the	spectroscopic characterization easier.
Xi Tauri a	spectroscopic and eclipsing triple star.
	spectroscopic methods for structural characterization
freely accessible, and contains extensive	spectroscopic data for organic compounds including that
mmonly used in fluorescence microscopy and	spectroscopic applications for selection of the excitati
	Spectroscopic observation from orbit indicates the prese
	Spectroscopic measurements have given an orbital period
IR	spectroscopic studies have demonstrated the existence of
Nu Scorpii A is itself a semi-detached	spectroscopic binary, having a fainter B-type companion
It is a	spectroscopic binary having a 113.8 day period, indicati
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.
The star e Serpentis (e Ser) is a	spectroscopic binary in the constellation of Serpens.
Pi Andromedae (π And, π Andromedae) is a	spectroscopic binary in the constellation Andromeda.
VV Corvi (VV Crv) is a close	spectroscopic binary in the Corvus constellation.
First discovered	spectroscopic binary in 1889 by an American astronomer E
Zeta Trianguli Australis (ζ TrA) is a	spectroscopic binary in the constellation Triangulum Aus
31 Camelopardalis is an eclipsing	spectroscopic binary in the constellation Camelopardalis
Wide Band Spectrometer (WBS) has	spectroscopic capabilities in a wide energy band from 3
anis Majoris (ζ CMa, ζ Canis Majoris) is a	spectroscopic binary in the constellation Canis Major.
However, more detailed	spectroscopic observations in 2005 appear to show that i
UT) was a space telescope designed to make	spectroscopic observations in the far-ultraviolet region
omedae was discovered to be a double-lined	spectroscopic binary in a series of spectra taken in 189
ve diseases and the use of microscopic and	spectroscopic methods in neurosciences (“neurophotonics”
s (τ CMa, τ Canis Majoris) is an eclipsing	spectroscopic binary in the constellation Canis Major an
Muterspaugh and M. Williamson at a robotic	spectroscopic telescope in Arizona, cf.).
He became interested in using	spectroscopic methods including nuclear magnetic resonan
Both visible and infrared	spectroscopic results indicate that Ixion's surface is a
NMR	spectroscopic experiments indicated close proximity of t
Despite this, chemical and	spectroscopic testing indicates that the photograph is a
	Spectroscopic analysis indicates the possible presence o
ars to have an orbital period of 11 years;	spectroscopic evidence indicates a third companion of A
e closest approach to this resolution by a	spectroscopic neutron instrument type, namely the backsc
At the centre of the system is a	spectroscopic binary, Iota Serpentis A and B. These are
	Spectroscopic parallax is an astronomical method for mea
As an optical technique,	spectroscopic ellipsometry is non-destructive and contac
Magnetic resonance	spectroscopic imaging is a noninvasive imaging method th
An advantage of this	spectroscopic technique is that the ions can be detected
The orbit of a	spectroscopic binary is determined by making a long seri
tside of Virginia, however, a 1-m aperture	spectroscopic telescope is found in Georgia at the Hard
Although	spectroscopic evidence is consistent with a mass of 8 ±
A suspected	spectroscopic binary, it has now been resolved by speckl
Theta-1 Sagittarii is a	spectroscopic binary lying 617 light years from Earth.
They are a	spectroscopic binary, meaning the separation between the
The Rossiter-McLaughlin effect is a	spectroscopic phenomenon observed when either an eclipsi
erally obtained empirically from gas-phase	spectroscopic studies of atoms.
Donati was also a pioneer in the	spectroscopic study of the stars and the sun.
RI scanner for functional, structural, and	spectroscopic studies of humans and animals.
vae, he has also worked extensively on the	spectroscopic studies of Active Galactic Nuclei
This instrument had a	spectroscopic range of 82.5 to 185 nms, and a spectral r
FOS was designed to make	spectroscopic observations of astrophysical sources from
The	spectroscopic assignment of these states follows the Ryd
s contributions to Astronomical Physics by	spectroscopic observations of eclipses, solar pre-eminen
The	spectroscopic properties of Proton-sponge are very inter
67 jointly with William Huggins, for their	spectroscopic study of the composition of stars.
In 1895, his	spectroscopic study of the rings of Saturn revealed that
of predictive models for use in real-time	spectroscopic analysis of materials.
ae (V415 Car or A Carinae) is an eclipsing	spectroscopic binary of the Algol type in the constellat
trophysics (ASCA) for a spatially resolved	spectroscopic analysis of Abell 2256 over the energy ban
y Notices Roy Astron Soc, vol lxv, 1905); '	Spectroscopic Observations of the Great Sunspot (Februar
	Spectroscopic methods on a cellular and molecular level
The Hubble Space Telescope took STIS/UV	spectroscopic observations on May 3, 2010.
uting is an approach to the development of	spectroscopic instruments, particularly for industrial a
ject was known as Small Main-belt Asteroid	Spectroscopic Survey, Phase II or SMASSII, which built o
resolved Pismis 24-1SW and the unresolved	spectroscopic binary Pismis 24-1NE.
Gamma rays detected in a	spectroscopic system produce peaks in the spectrum.
ame logic follows to explain the identical	spectroscopic results provided by the hydrogen atoms on
Biochemical and Mass	Spectroscopic analysis revealed that this pyroptosome is
A	spectroscopic analysis showed it to have a composition v
effects of weak gravitational lensing) and	Spectroscopic All Sky Cosmic Explorer (SPACE, to measure
Modern	spectroscopic and spectrometric techniques have since su
θ1 Crucis (θ1 Cru, Theta1 Crucis) is a	spectroscopic binary star in the constellation Crux.
θ2 Crucis (θ2 Cru / Theta2 Crucis) is a	spectroscopic binary star in the constellation Crux.
Alpha Equulei is a unique	spectroscopic binary star consisting of two components.
Pi4 Orionis (π4 Ori, π4 Orionis) is a	spectroscopic binary star in the constellation Orion.
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
(ε Her, ε Herculis) is a fourth-magnitude	spectroscopic binary star in the constellation Hercules.
ei is a triple star system consisting of a	spectroscopic double star with a wider companion.
Gliese 678 is a	spectroscopic binary star system approximately 60 light-
HD 176051 is a	spectroscopic binary star system located approximately 4
It is also a	spectroscopic binary star with a period of almost 273 da
omedae (Eta And, η Andromedae, η And) is a	spectroscopic binary star in the constellation of Androm
Atik is a	spectroscopic binary star consisting of a spectral type
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
Tau Puppis is also a	spectroscopic binary star system in which the multiple c
Theta Cephei is a white	spectroscopic binary star, located about 135 light-years
The star has been found to be a	spectroscopic binary star.
Carl Vogel, Pickering discovered the first	spectroscopic binary stars.
using a	spectroscopic technique, such as infrared spectroscopy,
ion to the new equilibrium is monitored by	spectroscopic probes such as fluorescence or less freque
	Spectroscopic studies suggest that Eunomia has regions w
In 1898 this system was reported to be a	spectroscopic binary system, with an orbital period of 2
This is a single-lined	spectroscopic binary system.
rferometer was used to resolve a number of	spectroscopic binary systems, including Alpha Andromedae
llipsometry (MOGE) is an advanced infrared	spectroscopic ellipsometry technique for studying free c
of the system components, A and B, form a	spectroscopic binary that completes an orbit every 76 ye
Linear dichroism (LD) is a	spectroscopic technique that is primarily used to study
at showed radio loud quasars have distinct	spectroscopic signatures that depend on their orientatio
solution Transmission) is a compilation of	spectroscopic parameters that a variety of computer code
In all three	spectroscopic methods, the sample usually needs to be pr
binary star, whose two components are both	spectroscopic binaries themselves, making a four-star sy
the subject of numerous X-ray diffraction,	spectroscopic and theoretical studies.
	Spectroscopic observations through 2007 indicate that it
He identified this gas by	spectroscopic methods to be nitrogen.
second per century, which corresponds from	spectroscopic observations to 20-30 km−1).
imation of this coupling provides a direct	spectroscopic route to the distance between nuclei and h
The	spectroscopic radial velocity is radial component of the
adial velocity most commonly refers to the	spectroscopic radial velocity.
B's	spectroscopic companion was discovered in 1989, and that
This is a	spectroscopic binary, which means that the individual co
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
Kappa Velorum is	spectroscopic binary which is classified as a blue-white
Kappa Arietis is a	spectroscopic binary which is classified as a white A-ty
The presence of water ice is supported by	spectroscopic observations, which have revealed crystall
Reflectance difference spectroscopy is a	spectroscopic technique which measures the difference in
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 whose two components are separated
It is a	spectroscopic binary whose components have magnitudes of
It is a	spectroscopic binary, whose components are separated by
Nu Andromedae is	spectroscopic binary whose components are a blue-white B
It is a	spectroscopic binary with an orbital period of 143.6065
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.
It is a	spectroscopic binary with a faint class-G companion.
Beta Cephei is a triple star comprising a	spectroscopic binary with a magnitude 8 optical companio
omponent, Iota Trianguli Australis A, is a	spectroscopic binary with a mean apparent magnitude of +
It is a	spectroscopic binary with components that are too close
The system consists of a	spectroscopic binary with a yellow G-type supergiant and
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
his work in development of ultrasensitive	spectroscopic methods with applications in trace gas det

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