「Binary」の共起表現(1語左で並び替え)5ページ目

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共起表現

「Binary」の共起表現一覧(1語左で並び替え)5ページ目

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n computer science, a left child-right sibling	binary tree is a binary tree representation of a k-ar
Using a simple	binary heap data structure and an adjacency list repr
which is a convenient rate to use with simple	binary counter circuits.
A simple	binary tree of size 9 and height 3, with a root node
A dropfile is a simple	binary or text file used by a bulletin board system (
Given a simple,	binary component feed, analytical methods such as the
Various subsets of the sixteen	binary connectives (e.g.
s encoding is that the first VLQ has the sixth	binary digit reserved to indicate whether the encoded
809 Lundia is a small,	binary, V-type asteroid orbiting within the Flora fam
line graph construction of the three smallest	binary De Bruijn graphs is depicted below.
used in statistics and engineering for solving	binary classification problems when the underlying da
ts (from object-oriented programming), in some	binary or textual form, adhering to some interface de
or other multimedia objects, though sometimes	binary executable code is stored as a blob.
a And, η Andromedae, η And) is a spectroscopic	binary star in the constellation of Andromeda.
A suspected spectroscopic	binary, it has now been resolved by speckle interfero
It is a spectroscopic	binary, which means it is a binary star with componen
discovered to be a double-lined spectroscopic	binary in a series of spectra taken in 1899 and 1900.
17 Leporis (17 Lep) is a spectroscopic	binary star in the constellation of Lepus.
Carinae (a Car, a Carinae) is a spectroscopic	binary in the constellation Carina.
It is a suspected spectroscopic	binary, although this has not been confirmed.
Theta-1 Sagittarii is a spectroscopic	binary lying 617 light years from Earth.
cis (θ1 Cru, Theta1 Crucis) is a spectroscopic	binary star in the constellation Crux.
he star e Serpentis (e Ser) is a spectroscopic	binary in the constellation of Serpens.
ei is a triple star comprising a spectroscopic	binary with a magnitude 8 optical companion.
It is a spectroscopic	binary whose components have an orbital period of 10.
tarii (υ Sgr, υ Sagittarii) is a spectroscopic	binary star system in the constellation Sagittarius.
It is a spectroscopic	binary whose components have an orbital period of 402
Rho Tucanae is a spectroscopic	binary composed of two yellow-white F-type main seque
e of 5".1 while it may also be a spectroscopic	binary.
They are a spectroscopic	binary, meaning the separation between the two is ver
The primary is a spectroscopic	binary, and its close companion completes one orbit e
It is a spectroscopic	binary with an orbital period of 143.6065 days.
medae (π And, π Andromedae) is a spectroscopic	binary in the constellation Andromeda.
It is a spectroscopic	binary and has a companion located 0.12 arcseconds aw
Nu Andromedae is spectroscopic	binary whose components are a blue-white B-type main
Secondary, Σ 1694 B is a spectroscopic	binary both A-type main sequence star.
It is a spectroscopic	binary whose two components are separated by 0.1 arcs
It is a spectroscopic	binary, and the two subcomponents have apparent magni
itself has been identified as a spectroscopic	binary star system; this means that Delta Muscae was
Chi Aurigae is a spectroscopic	binary which is classified as a blue-white B-type sup
104 Aqr A is a spectroscopic	binary and is suspected to be variable.
The system consists of a spectroscopic	binary with a yellow G-type supergiant and a white A-
was used to resolve a number of spectroscopic	binary systems, including Alpha Andromedae, Phi Cygni
Theta Aquilae is a spectroscopic	binary classified as a blue-white B-type giant with a
Iota Trianguli Australis A, is a spectroscopic	binary with a mean apparent magnitude of +5.28.
Herculis) is a fourth-magnitude spectroscopic	binary star in the constellation Hercules.
VV Corvi (VV Crv) is a close spectroscopic	binary in the Corvus constellation.
Lambda Andromedae is a spectroscopic	binary with an orbital period of 20.52 days.
It is a spectroscopic	binary with an orbital period of 134 days.
ar or A Carinae) is an eclipsing spectroscopic	binary of the Algol type in the constellation of Cari
is (θ2 Cru / Theta2 Crucis) is a spectroscopic	binary star in the constellation Crux.
his star is suspected of being a spectroscopic	binary, although this has not yet been confirmed.
τ Canis Majoris) is an eclipsing spectroscopic	binary in the constellation Canis Major and the brigh
Theta Cephei is a white spectroscopic	binary star, located about 135 light-years from Earth
e of approximately 5.15 and is a spectroscopic	binary star which consists of two giant stars, each w
Iota Arietis is a spectroscopic	binary classified as a yellow G-type supergiant with
Component A is a spectroscopic	binary.
stem components, A and B, form a spectroscopic	binary that completes an orbit every 76 years.
HD 37017 is a spectroscopic	binary.
Lambda Virginis is a spectroscopic	binary.
IU Aurigae is a spectroscopic	binary.
First discovered spectroscopic	binary in 1889 by an American astronomer Edward Picke
EZ Aquarii AC is a spectroscopic	binary.
Sigma Aquilae is an eclipsing spectroscopic	binary.
It is a spectroscopic	binary with components that are too close together to
rpii A is itself a semi-detached spectroscopic	binary, having a fainter B-type companion separated b
th optical telescopes, forming a spectroscopic	binary.
, Pickering discovered the first spectroscopic	binary stars.
Alpha Equulei is a unique spectroscopic	binary star consisting of two components.
Trianguli Australis (ζ TrA) is a spectroscopic	binary in the constellation Triangulum Australe.
422 Monocerotis or HR 2422) is a spectroscopic	binary at a distance of around 6600 light-years.
It is also a spectroscopic	binary, and is composed of two stars with apparent ma
Ursae Minoris A, is an eclipsing spectroscopic	binary.
is (ζ CMa, ζ Canis Majoris) is a spectroscopic	binary in the constellation Canis Major.
ponent, Epsilon Volantis A, is a spectroscopic	binary.
Gliese 678 is a spectroscopic	binary star system approximately 60 light-years away
This is a spectroscopic	binary, which means that the individual components ha
Kappa Velorum is spectroscopic	binary which is classified as a blue-white B-type sub
r, Kappa Pegasi B, is actually a spectroscopic	binary, with the components designated Kappa Pegasi B
This is a single-lined spectroscopic	binary system.
ar has also been identified as a spectroscopic	binary with a period of 494 days, but the companion h
3 Camelopardalis is a spectroscopic	binary in the constellation Camelopardalis.
At the centre of the system is a spectroscopic	binary, Iota Serpentis A and B. These are both white
SBC7 is an acronym for Spectroscopic	Binary 7th Catalogue.
It is a spectroscopic	binary whose components have magnitudes of +4.1 and +
rionis (π4 Ori, π4 Orionis) is a spectroscopic	binary star in the constellation Orion.
HD 176051 is a spectroscopic	binary star system located approximately 49 light yea
Atik is a spectroscopic	binary star consisting of a spectral type B1 giant an
It is a spectroscopic	binary having a 113.8 day period, indicating that its
It is also a spectroscopic	binary star with a period of almost 273 days and an e
Tau Puppis is also a spectroscopic	binary star system in which the multiple companions w
The orbit of a spectroscopic	binary is determined by making a long series of obser
The star has been found to be a spectroscopic	binary star.
This star is a spectroscopic	binary, and the primary is also a Beta Cephei variabl
It consists of a spectroscopic	binary and a third component.
It is a spectroscopic	binary, whose components are separated by 0.176 arcse
Pismis 24-1SW and the unresolved spectroscopic	binary Pismis 24-1NE.
It is a spectroscopic	binary with a faint class-G companion.
1 Camelopardalis is an eclipsing spectroscopic	binary in the constellation Camelopardalis.
12 Camelopardalis is a spectroscopic	binary in the constellation Camelopardalis.
Kappa Arietis is a spectroscopic	binary which is classified as a white A-type main seq
nation the orbital period of A's spectroscopic	binary difficult.
V373 Cas is a spectroscopic	binary in the constellation Cassiopeia.
this system was reported to be a spectroscopic	binary system, with an orbital period of 280.55 days.
nion, which would make Electra a spectroscopic	binary.
k-red crystalline solid is the smallest stable	binary rhodium carbonyl.
Ir4(CO)12, which is the most common and stable	binary carbonyl of iridium.
ough draft, before the eventual move to stable	binary programs.
lsations of the transient neutron star/Be star	binary 4U 0115+63., leading to determination of its o
ument to study chromospherically active stars,	binary stars, and pre-main sequence stars, for exampl
A translator using static	binary translation aims to convert all of the code of
and 0.8.x releases which was meant to stay	binary compatible within those release series.
He extensively studied	binary stars and was recognized for this work.
l fellow and part-time faculty member studying	binary systems at the Dunlap Observatory, Bolton obse
This strategy of subverting	binary oppositions (such as contestation vs. consensu
l too, but this doesn't go that far... Tarquin	Binary 18:01, 9 March 2007 (UTC)
h is Stoke Newington Church Street...) Tarquin	Binary 12:48, 1 March 2007 (UTC)
Done, see what you think... Tarquin	Binary 20:38, 26 February 2007 (UTC)
e doesn't mention the museum, oddly... Tarquin	Binary 15:32, 28 February 2007 (UTC)
Tarquin	Binary 20:04, 26 February 2007 (UTC)
Tarquin	Binary 14:36, 29 August 2005 (UTC)
Tarquin	Binary 15:04, 29 August 2005 (UTC)
Tarquin	Binary 15:52, 26 January 2006 (UTC)
y used plant transformation vectors are termed	binary vectors because of their ability to replicate
al, were based on decimal notation rather than	binary; as Kitz himself stated at a symposium "no bin
ould still occur, merely that it accepted that	binary traffic was the norm on that port, and not giv
iatory chemical capability in the form of that	binary chemical weapons program.
is requirement can be rephrased by saying that	binary meets preserve binary joins.
pic companion was discovered in 1989, and that	binary has a period of 33.01 years.
The	binary search algorithm is a method of searching an o
rii (V4134 Sgr) is a low mass star so that the	binary 4U 1755-33 is a low-mass X-ray binary (LMXB).
The method is also called the	binary search method and is similar to the computer s
on) between processes is represented using the	binary communications operator, .
t of the separation step is retained, i.e. the	binary phase-envelope diagram (boiling-point curve) m
Essentially the concept of the	binary opposition is prompted by the Western tendency
are now known to have unusual properties: the	binary asteroid with equal components 90 Antiope and
Unlike the	binary integer significand version, where the exponen
MAGX, a version of Linux, but instead runs the	Binary Runtime Environment for Wireless operating sys
Both components of the	binary star are a white A-type main sequence dwarfs.
days, which is also the orbital period of the	binary.
running FastContact online or downloading the	binary was set up by P. Christoph Champ in July 2005.
You can download the	binary ZIP package which contains only the main execu
Both components of the	binary star are yellow-white F-type stars and they ha
The	binary digits in the map represent the function's out
he original tree is made its left child in the	binary tree, and its nearest sibling to the right in
g subtitle is "0100100001101001", which is the	binary representation of the ASCII encoding of the wo
It was also the home for the	Binary Chemical Weapons Facility.
in rinfabate (trade name: Iplex), which is the	binary complex of recombinant human IGF-1 (rhIGF-1) a
The	binary format is widely used within Esri programs, su
gious nationalism may articulate itself as the	binary of secular nationalism.
The	binary Golay code, along with the ternary Golay code,
The	binary star system consists of a white dwarf closely
Plato, because “…Plato's Gorgias agrees to the	binary opposition knowledge vs. opinion” (82).
ltimately fall onto the neutron star as in the	binary system Cen X-3.
limb darkening in distant stars, constrain the	binary star population, and constrain the structure o
in certain variations in orbital period of the	binary system.
The primary component of the	binary system is suspected to host a substellar compa
ting Psi1 Draconis A, primary component of the	binary system.
FCRAO labs contributed to the discovery of the	binary pulsar system PSR B1913+16 by Joseph Taylor an
As in the case of a white-dwarf donor, the	binary orbit is expected to 'bounce' and start expand
One of the components of the	binary is also classified as a Gamma Doradus type var
s a finitely axiomatized generalization of the	binary relation example, but there exist interesting
The	binary has an apparent magnitude of +4.53 and an orbi
each indicator there was a board decoding the	binary code sent by the main board.
For example, the	binary relation "the product of x and y is even" is r
If the	binary relation is antisymmetric, transitive and also
The	binary system is an RS Canum Venaticorum variable and
the galaxy, like Eta Carinae, HD 93250 and the	binary HD 93129.
The	binary star AB Doradus B orbits the primary at an ave
The second, smaller star of the	binary orbits very closely and may even have been eng
f 15.4 hours, which roughly indicates that the	binary is very close - the separation being of the or
an exoplanet orbiting around HD 195019 in the	binary star system.
The most massive stars in the cluster are the	binary star system BD+31°643, which has a combined sp
he source, and were therefore evidence for the	binary nature of Centaurus X-3.
d Equilibrium and Excess Enthalpy Data for the	Binary Systems Water + Sulfolane and Methanol + N-Met
The	Binary Space blog page follows the game's development
Orbiting the	binary star, at a distance of 36 arcseconds, roughly
nt fractions in the range -1 ≤ x < 1, i.e. the	binary point was immediately to the right of the sign
ions support the Fast Infoset standard for the	binary encoding of the XML infoset.
are the	binary exotoxins.
The orbital period of the	binary is 1567.7 days and the two components are sepa
1 in the significand of normal values for the	binary formats.
The	binary system at the center of the nebula was first d
The	binary star also has two optical companions, the 12th
The	binary system consists of two red dwarf stars orbitin
with only four basic symbols representing the	binary digits one and zero and open and close bracket
by injecting aspect-related code back into the	binary.
tric Arcade Style Racing Game developed by The	Binary Mill for the iOS platform.
The	binary star revolves around its common centre of mass
nown as nitrogen pentoxide, N2O5 is one of the	binary nitrogen oxides, a family of compounds that on
ejected Army requests for authorization of the	binary chemical weapons program.
2006, the Keck Observatory announced that the	binary Trojan asteroid 617 Patroclus, and possibly la
instead to the generated code size or even the	binary file size.
mother of Gottfried Leibniz, discoverer of the	binary numeral system and one of the inventors of cal
x and its successors can take advantage of the	binary compatibility with real mode to run many Windo
ve than Jupiter and is located 8.6 AU from the	binary.
Just as binomial heaps are based on the	binary number system, skew binary heaps are based on
The	binary nature of this asteroid was suggested from rad

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共起表現

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「Binary」の共起表現一覧(1語左で並び替え)5ページ目