「Binary」の共起表現一覧(2語右で並び替え)4ページ目
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The game is available in | binary distribution only (no sources) for both system |
The following | binary (containing only Cs and O) oxides of caesium a |
d as nullary (no operands), unary (1 operand), | binary (2 operands), ternary (3 operands) etc. |
on) between processes is represented using the | binary communications operator, . |
relevant logic, the implication operator is a | binary modal operator, and negation is usually taken |
i (a DQ Herculis variable), the low-mass X-ray | binary V2293 Ophiuchi, 80 ROSAT visibly dark X-ray so |
ese stars rotate particularly fast, have close | binary companions, or are very young. |
ention used to identify the bit positions in a | binary number or a container for such a value. |
riod of 0.1 s or 0.2 s, which corresponds to a | binary "0" or "1". |
1. | binary acids or hydracids and 2. oxoacids that contai |
extual source file that can be compiled into a | binary file or one of two text representations. |
as an alternative to | binary 0 or 1. |
that describes the symmetries of the infinite | binary tree or Cantor set. |
not necessarily conform to a specific hardware | binary interface, or instruction set, can be either r |
echniques work best for samples of homogeneous | binary materials or uniform surface layers, while ele |
Discrete outcomes, such as | binary decisions or qualitative data restricted to a |
iriKiri/KAG is expandable with plugins in both | binary (.dll) or its own script format. |
cal or geochemical system, a solvus is a line ( | binary system) or surface (ternary system) on a phase |
The two | binary systems orbit around each other once every 818 |
The | binary is orbited by a third component, Epsilon Ursae |
instrumental music track by British trance act | Binary Finary originally released in the year 1998. |
agery suggests that Annefrank may be a contact | binary, although other possible explanations exist fo |
l elements are sent in sequence to represent a | binary one; otherwise it is interpreted as binary zer |
Davis (2000) says that Turing built a | binary multiplier out of electromechanical relays (p. |
olatile solid is a rare example of a molecular | binary metal oxide, the other examples being RuO4, Os |
nown as nitrogen pentoxide, N2O5 is one of the | binary nitrogen oxides, a family of compounds that on |
You can download the | binary ZIP package which contains only the main execu |
the set of variables, and associated with each | binary element pair |
Mu Herculis A and the | binary itself pair B-C are separated by 286 AUs. |
Binary space partitioning (BSP) is a method for recur | |
e and had some fun implementing a BSP library ( | Binary Space Partitioning). |
he is known for her work with Mike Paterson on | binary space partitioning, her work with Dan Greene o |
Here, | binary signals pass along nine ordinary transmission |
etermine weight percentages of each phase of a | binary equilibrium phase diagram. |
2001 QW322 is a | binary minor planet and cubewano in the Kuiper belt. |
limb darkening in distant stars, constrain the | binary star population, and constrain the structure o |
is requirement can be rephrased by saying that | binary meets preserve binary joins. |
e language implementation problem, see Fragile | binary interface problem. |
used in statistics and engineering for solving | binary classification problems when the underlying da |
Bsdiff is a | binary diff program using suffix sorting. |
a technology allowing common "shrink wrapped" | binary application programs to be distributed for use |
Net4j based | binary application protocol |
NT LAN Manager Security Support Provider) is a | binary messaging protocol used by the Microsoft Secur |
In 1974, Hulse and Taylor discovered | binary pulsar PSR B1913+16, which is made up of a pul |
Popular theories for the formation of | binary millisecond pulsars require mass transfer onto |
the average flux, which is often observed from | binary X-ray pulsars. |
He is known for predicting | binary radio pulsars. |
"The Extreme Kuiper Belt | Binary 2001 QW322". |
In mathematics, a | binary relation R on a set X is Euclidean (sometimes |
Suppose X and Y are arbitrary sets and a | binary relation R over X and Y is given. |
In mathematics, a | binary relation R over a set X is transitive if whene |
s said to be recursive if there is a recursive | binary relation R that well-orders a subset of the na |
(often shortened to ancestral) of an arbitrary | binary relation R is defined below. |
In mathematics, a | binary relation R over a set X is symmetric if it hol |
In mathematics, a | binary relation R on a set X is antisymmetric if, for |
In mathematics, the reflexive closure of a | binary relation R on a set X is the smallest reflexiv |
In mathematics, the symmetric closure of a | binary relation R on a set X is the smallest symmetri |
In mathematics, a transitive reduction of a | binary relation R on a set X is a minimal relation R' |
currence might cause compatibility issues with | binary news readers that cannot address post counts s |
equivalent to monadic first order logic with a | binary equality relation. |
FBReader has since had | binary packages released for many mobile device platf |
Version 2.26 in universal | binary was released on the 17th of March 2009, requir |
As a result, | binary package repositories are a transparent optimiz |
A cladogram in the form of an unrooted | binary tree, representing the similarities and evolut |
s (e.g. that of double planet, but not that of | binary star) require that this center of mass is not |
s encoding is that the first VLQ has the sixth | binary digit reserved to indicate whether the encoded |
The | binary star revolves around its common centre of mass |
tractly defined as commutative and associative | binary operations satisfying an idempotency law. |
t of a group in the modern way-as a set with a | binary operation satisfying certain laws. |
ersion of WebKit instead of WebCore, universal | binary support, saving to web archive, support for us |
Elaborate schemes allowed users to download | binary files, search gopherspace, and interact with d |
See my other posts a | Binary compatibility section of the discussion for th |
gious nationalism may articulate itself as the | binary of secular nationalism. |
For observing | binary stars, see de Sitter double star experiment. |
each indicator there was a board decoding the | binary code sent by the main board. |
structs needed for systems programming such as | binary input-output, separate compilation, variables |
The system consists of two | binary pairs separated by 5.3 arcminutes. |
Alongside with | binary variables, sequentions are also forming compon |
At the centre of the system is a spectroscopic | binary, Iota Serpentis A and B. These are both white |
running FastContact online or downloading the | binary was set up by P. Christoph Champ in July 2005. |
Unlike the | binary integer significand version, where the exponen |
300 X-1 is a new kind of Wolf-Rayet black hole | binary system similar to the confirmed such system IC |
on speed, higher memory consumption and larger | binary program size. |
instead to the generated code size or even the | binary file size. |
ng the number of bits which are set to 1 in a ( | binary) number, sometimes called the population funct |
ginal discovery of this periodically pulsating | binary X-ray source occurred in November 1971. |
This is a major advantage over | binary or source auditing, or even fuzzing's close co |
Binary and source code distributions are available. | |
bution License and is freely available in both | binary and source code form. |
s black hole candidate and 2000-2001 transient | binary X-ray source located in the constellation Ara. |
different strong accreting, pulsing, eclipsing | binary X-ray source Vela X-1, also known as 4U 0900-4 |
Although it was observed to be | binary by speckle interferometry in 1985, subsequent |
It is a wide | binary of spectral class B stars, each of magnitude 4 |
installed on Linux and FreeBSD using the Intel | Binary Compatibility Standard (ibcs2) support library |
A | binary companion star was detected in 2007 at the Gem |
LCGT will detect chirp waves from | binary neutron star coalescence at 240 Mpc away with |
As an eclipsing | binary, the star would undergo regular changes in bri |
Delta Hydrae is a | binary double star, located about 180 light-years fro |
arfs, and observational studies of interacting | binary collapsed stars. |
etical plates required for the separation of a | binary feed stream by a fractionation column that is |
Page description languages are textual or | binary data streams. |
n important role when it comes to non-mergable | binary files such as graphic assets. |
quasi-ordering (i.e., a reflexive, transitive | binary relation) such that any infinite sequence of e |
duced as a result of mixing two chemicals as a | binary liquid, such as plastic foams and some explosi |
The primary component of | binary is suspected to host an extrasolar planet. |
V404 Cygni is a | binary star system consisting of a black hole with a |
BG Geminorum is long period eclipsing | binary star system which contains a K0 I secondary st |
Beta Pyxidis (β Pyx) is a | binary star system located in the constellation Pyxis |
tarii (υ Sgr, υ Sagittarii) is a spectroscopic | binary star system in the constellation Sagittarius. |
ributions to the study of Gas Giant Planet and | binary star system formation. |
This | binary star system consists of two closely spaced low |
52 Cygni is a | binary star system in the Veil Nebula. |
Zeta Herculis (ζ Her, ζ Herculis) is a | binary star system in the constellation Hercules. |
The | binary star system consists of a white dwarf closely |
ative solution is that neutron star mergers (a | binary star system of two neutron stars that collide) |
SAO 49986 and SAO 49982 form a | binary star system in the constellation Cygnus. |
FCRAO labs contributed to the discovery of the | binary pulsar system PSR B1913+16 by Joseph Taylor an |
Circinus X-1 is an X-ray | binary star system that includes a neutron star. |
ts theorize that the star was ejected out of a | binary star system approximately 80 million years ago |
eta Cygni (ζ Cyg) and CCDM J21129+3014B form a | binary star system in the constellation Cygnus, appro |
ned that the craft came from the Zeta Reticuli | binary star system and that extraterrestrials have be |
This is an interacting | binary star system consisting of a white dwarf primar |
Temperature control was achieved using a | binary gas-liquid system and hemispherical radiators |
Artist's conception of a | binary star system with one black hole and one main s |
17 Lyrae is a | binary star system in the constellation Lyra, approxi |
Lambda Ophiuchi (λ Oph, λ Ophiuchi) is a | binary star system in the constellation Ophiuchus. |
The most massive stars in the cluster are the | binary star system BD+31°643, which has a combined sp |
Components A and B form a close | binary star system with a short orbital period of onl |
-9 represents the spectacular “last gasp” of a | binary star system at the nebula's center. |
ese 250 (also known as 88 G. Monocerotis) is a | binary star system with a relatively high proper moti |
Delta1 Lyrae (δ1 Lyr) is a | binary star system in the constellation Lyra, approxi |
HD 142022 is a | binary star system located in the southernmost conste |
641 Sagittarii (V4641 Sgr) is a variable X-ray | binary star system in the constellation Sagittarius. |
HR 4458 (289 G. Hydrae) is a | binary star system in the constellation Hydra. |
ataclysmic variable star consisting of a close | binary star system in which one of the components is |
phei, also known as HD 208816, is an eclipsing | binary star system located in the constellation Cephe |
Gliese 752 was not known to be a | binary star system until the discovery of a small dim |
HD 197488, also known as BD +45°3245, forms a | binary star system in the constellation Cygnus. |
UX Tauri, abbreviated as UX Tau, is a | binary star system approximately 450 light-years away |
mother of Gottfried Leibniz, discoverer of the | binary numeral system and one of the inventors of cal |
Alpha Columbae is a | binary star system CCDM J05396-3404. |
The | binary numeral system is invented by mathematician Ba |
Beta Lyrae (β Lyr, β Lyrae) is a | binary star system approximately 882 light-years away |
9733, also catalogued as V452 Vulpeculae, is a | binary star system approximately 63 light-years away |
Phi Piscium (φ Psc) is a | binary star system approximately 380 light years away |
η Oph is actually a | binary star system that is difficult to resolve in am |
Gliese 678 is a spectroscopic | binary star system approximately 60 light-years away |
HD 178911 is a | binary star system in the constellation Lyra. |
NGC 3603-A1 is a massive, double-eclipsing | binary star system located in NGC 3603, about 20,000 |
OGLE-TR-122 is a | binary stellar system containing one of the smallest |
OGLE-TR-123 is a | binary stellar system containing one of the smallest |
Tau4 Eridani is a | binary star system consisting primarily of Class M co |
HD 16760 is a | binary star system approximately 150 light-years away |
HD 176051 is a spectroscopic | binary star system located approximately 49 light yea |
HD 211415 is a | binary star system in the constellation Grus. |
Tau Puppis is also a spectroscopic | binary star system in which the multiple companions w |
Gliese 505 is a | binary star system located thirty-seven light-years a |
HR 4796 is a | binary star system approximately 220 light-years away |
Delta Equulei is a | binary star system about 60 light years away, with co |
94 Ceti (HD 19994) is a | binary star system approximately 73 light-years away |
171301 and BD+30°3223B are two components of a | binary star system in the constellation Lyra, approxi |
PSR B1620-26 is a | binary star system approximately 12,400 light-years a |
Recent measurements indicate that the | binary star system has an age of several billion year |
35 Piscium is a | binary star system in the constellation Pisces. |
4U 0614+091 is an X-ray | binary star system which features a neutron star and |
49 Cassiopeiae is a | binary star system in the constellation Cassiopeia, a |
Mu Cassiopeiae (μ Cas, μ Cassiopeiae) is a | binary star system in the constellation Cassiopeia. |
Tau Cygni (τ Cyg) is a | binary star system in the constellation Cygnus, appro |
HD 222501 and HD 222502 are two stars in a | binary star system, separated from each other by abou |
lculate the angular distance in arcseconds for | binary star system, extrasolar planets, solar system |
ADS 16402 is a | binary star system, composed of two sun-like stars lo |
HD 93205 is a | binary stellar system, in the Carina Nebula (NGC 3372 |
Just as binomial heaps are based on the | binary number system, skew binary heaps are based on |
ers, was determined to be a previously unknown | binary star system. |
e formed from the dust that is spewed out of a | binary star system. |
idence suggesting that Eta Leonis is part of a | binary star system. |
It is thought that the star may, in fact, be a | binary star system. |
It may or may not be a close | binary star system. |
an exoplanet orbiting around HD 195019 in the | binary star system. |
is a double star once thought to be part of a | binary star system. |
the TrES-2 system (along with two others) is a | binary star system. |
T-P-1 is the dimmer component of the ADS 16402 | binary star system. |
Meissa is actually a | binary star system. |
nd distances, confirming that they form a wide | binary star system. |
It is believed to be a | binary star system. |
tion when it receives a distress signal from a | binary star system. |
aked eye to be a single star, it is actually a | binary star system. |
panion star was detected in 1894 making this a | binary star system. |
itself has been identified as a spectroscopic | binary star system; this means that Delta Muscae was |
and Messier 60, these bright spots are due to | binary star systems of black holes and neutron stars |
lizes in cataclysmic variable stars, which are | binary star systems that periodically undergo energet |
lescope and is used for research (primarily of | binary star systems) by the Fairfield County Astronom |
ins several X-ray sources, thought to be close | binary star systems, as well as millisecond pulsars i |
f graph is a graphical plot of error rates for | binary classification systems, plotting false reject |
are low, and poor mixing is achieved for most | binary solvent systems, which makes this technique bo |
have been posited to explain the formation of | binary asteroid systems. |
They are also called high size ratio | binary asteroid systems. |
An unrooted | binary tree T may be transformed into a full rooted b |
e data variables, while the output is a set of | binary signals taken for input by the FSM-block. |
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