AI & ChatGPT searches , social queries for BINARY PULSAR
Search references for BINARY PULSAR. Phrases containing BINARY PULSAR
See searches and references containing BINARY PULSAR!
Search references for BINARY PULSAR. Phrases containing BINARY PULSAR
See searches and references containing BINARY PULSAR!BINARY PULSAR
Two pulsars orbiting each other
A binary pulsar is a pulsar with a binary companion, often a white dwarf or neutron star. (In at least one case, the double pulsar PSR J0737-3039, the
Binary_pulsar
Type of neutron star with beams of radiation
very useful tools for astronomers. For example, observations of a pulsar in a binary neutron star system were used to indirectly confirm the existence
Pulsar
Pulsar in the constellation Aquila
Hulse–Taylor pulsar (known as PSR B1913+16, PSR J1915+1606 or PSR 1913+16) is a binary star system composed of a neutron star and a pulsar which orbit
Hulse–Taylor_pulsar
Collapsed core of a massive star
pulsars or "accretion-powered pulsars": a class of X-ray binaries Low-mass X-ray binary pulsars: a class of low-mass X-ray binaries (LMXB), a pulsar with
Neutron_star
Aspect of relativity in physics
gravitational waves have since then been observed, first indirectly using binary-pulsar observations and, since 2015, directly through dedicated observatories
Gravitational_wave
Double pulsar in the constellation Puppis
double pulsar. It consists of two neutron stars emitting electromagnetic waves in the radio wavelength in a relativistic binary system. The two pulsars are
PSR_J0737−3039
Binary pulsar–neutron star system in the constellation Vulpecula
PSR J1946+2052 is a short-period binary pulsar system located 11,000–14,000 light-years (3,500–4,200 pc) away from Earth in the constellation Vulpecula
PSR_J1946+2052
Astronomical objects
CXJ0110-7211 Vela X-1 4U 0352+309 Bursting Pulsar Vela Junior LMC N49 Intermediate-mass X-ray binary High-mass X-ray binaries Centaurus X-3 Circinus X-1 GX 301-2
List_of_neutron_stars
Gravitational-wave astronomy technique
A pulsar timing array (PTA) is a set of galactic pulsars that is monitored and analyzed to search for correlated signatures in the pulse arrival times
Pulsar_timing_array
Pulsar in the constellation Pictor
of only two pulsars to have the full three-dimensional orientation of its orbit determined. Optical observations indicate that the binary companion of
PSR_J0437−4715
Hulse, Joseph Hooton Taylor Jr. and others studied the behaviour of binary pulsars experiencing much stronger gravitational fields than those found in
Tests_of_general_relativity
Canadian astronomer
University of British Columbia. She studies pulsars and their companions as a way to study binary pulsar evolution, pulsar instrumentation and polarimetry, and
Ingrid_Stairs
Theory of gravitation as curved spacetime
is not the case for a close binary pulsar, a system of two orbiting neutron stars, one of which is a pulsar: from the pulsar, observers on Earth receive
General_relativity
Pulsar with a rotational period less than about 10 milliseconds
companion star in a close binary system. For this reason, millisecond pulsars are sometimes called recycled pulsars. Millisecond pulsars are thought to be related
Millisecond_pulsar
2015 detection made by LIGO interferometers
been inferred only indirectly, via their effect on the timing of pulsars in binary star systems. The waveform, detected by both LIGO observatories, matched
First observation of gravitational waves
First_observation_of_gravitational_waves
Millisecond pulsar in the constellation Sagitta
The Black Widow pulsar (PSR B1957+20) is an eclipsing binary millisecond pulsar in the Milky Way. Discovered in 1988, it is located roughly 6,500 light-years
Black_Widow_pulsar
Astronomic function
pulses from a radio pulsar. A binary system is called a single-lined spectroscopic binary if the radial motion of only one of the two binary components can
Binary_mass_function
American physicist
survey for pulsars. It was this work that led to the discovery of the first binary pulsar. In 1974, Hulse and Taylor discovered binary pulsar PSR B1913
Russell_Alan_Hulse
Binary pulsar–neutron star system in the constellation Sagittarius
PSR J1930−1852 is a binary pulsar system, composed of a pulsar and a neutron star and orbiting around their common center of mass. Located 4,900 light-years
PSR_J1930−1852
Pulsar–white dwarf binary system in Taurus constellation
PSR J0348+0432 is a pulsar–white dwarf binary system in the constellation Taurus. It was discovered in 2007 with the National Radio Astronomy Observatory's
PSR_J0348+0432
Star in the constellation Sagittarius
The Bursting Pulsar (GRO J1744-28) is a low-mass x-ray binary with a period of 11.8 days. It was discovered in December 1995 by the Burst and Transient
Bursting_Pulsar
Class of astronomical objects that are X-ray sources
fraction of a second to as much as several minutes. An X-ray pulsar is a type of binary star system consisting of a typical star (stellar companion) in
X-ray_pulsar
Pulsar in the constellation Sagittarius
fastest-spinning pulsar known, at 716.35 Hz (times per second), or 42,981 revolutions per minute (1.3959 milliseconds). This pulsar was discovered by
PSR_J1748−2446ad
Massive millisecond pulsar in the Milky Way
PSR J0952−0607 is a massive millisecond pulsar in a binary system, located between 3,200–5,700 light-years (970–1,740 pc) from Earth in the constellation
PSR_J0952−0607
Random background of gravitational waves permeating the Universe
background from binary neutron-star and stellar mass binary black-hole mergers. An alternative means of observation is using pulsar timing arrays (PTAs)
Gravitational_wave_background
Millisecond pulsar in the constellation Aquila
PSR J1903+0327 is a millisecond pulsar in a highly eccentric binary orbit. The pulsar was discovered in an ongoing L-band (1.4 GHz) survey with the 305
PSR_J1903+0327
Binary star system in the globular cluster of Messier 4
system. One side regards the A/B convention of naming binary stars as having priority, so that the pulsar is PSR B1620−26 A, the white dwarf companion is PSR
PSR_B1620−26
Multi-spectrum pulsar in the constellation Vela
The Vela Pulsar (PSR J0835–4510 or PSR B0833–45) is a radio, optical, X-ray- and gamma-emitting pulsar associated with the Vela supernova remnant in the
Vela_Pulsar
Speed of electromagnetic waves
Abbott, B. P.; et al. (2017). "Gravitational Waves and Gamma-Rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A". The Astrophysical Journal
Speed_of_light
Radio telescope observatory in New South Wales, Australia
Pulsar Timing Array (IPTA), which also includes the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) and the European Pulsar Timing
Parkes_Observatory
Planets found orbiting pulsars
Pulsar planets are planets that are orbiting pulsars. The first such planets to be discovered were around a millisecond pulsar in 1992 and were the first
Pulsar_planet
European space mission to measure gravitational waves
observations of the decreasing orbital periods of several binary pulsars, such as the Hulse–Taylor pulsar. In February 2016, the Advanced LIGO project announced
Laser Interferometer Space Antenna
Laser_Interferometer_Space_Antenna
Flow of gas ejected from the upper atmosphere of a star
needed] Space portal Cosmic ray Cosmic wind Planetary wind Colliding-wind binary Pulsar wind nebula Galactic superwind Superwind Planetary nebula Asymptotic
Stellar_wind
Branch of astronomy using gravitational waves
waves came in 1974 from the observed orbital decay of the Hulse–Taylor binary pulsar, which matched the decay predicted by general relativity as energy is
Gravitational-wave_astronomy
American-Indian astronomer (born 1956)
graduate student. In 1986, he found the first optical counterpart of binary pulsars, while he was a Millikan Fellow at California Institute of Technology
Shrinivas_Kulkarni
Gravitational-wave detector in Italy
evidenced by the three-decade study of the binary pulsar 1913+16: the observed decrease of this binary pulsar's orbital period was in agreement with the
Virgo_interferometer
Gravitational-wave signal detected in 2017
years away. The wave was produced by the last moments of the inspiral of a binary pair of neutron stars, ending with their merger. It is the first GW detection
GW170817
Volunteer computing project
search effort is designed to find radio pulsars in tight binary systems. It is expected that there is one radio pulsar detectable from Earth in an orbital
Einstein@Home
Type of stellar collision
observed GW170817, a gravitational wave associated with the merger of a binary neutron star (BNS) system in NGC 4993, an elliptical galaxy in the constellation
Neutron_star_merger
Europe-US-Canada-India-Australian radio astronomy and cosmology collaboration
Pulsar Timing Array (IPTA) is a multi-institutional, multi-telescope collaboration of pulsar timing arrays (PTAs). It comprises the European Pulsar Timing
International Pulsar Timing Array
International_Pulsar_Timing_Array
Phenomenon in astrophysics
A pulsar kick is the name of the phenomenon that often causes a neutron star to move with a different, usually substantially greater, velocity than its
Pulsar_kick
Dutch astronomer (born 1940)
observed as binary radio pulsars. Van den Heuvel’s work provided the first evolutionary connection between X ray binaries and binary radio pulsars, elucidating
Ed_van_den_Heuvel
Gravitational wave observatory site
existence was indirectly confirmed in 1974, when observations of the binary pulsar PSR 1913+16 showed an orbital decay which matched Einstein's predictions
LIGO
Class of binary stars
X-ray pulsars (AMXPs) Ultracompact X-ray binaries (UCXBs) Intermediate-mass X-ray binaries (IMXBs) High-mass X-ray binaries (HMXBs) Be/X-ray binaries (BeXRBs)
X-ray_binary
Pulsar in the constellation of Musca
PSR J1141−6545 is a pulsar in the constellation of Musca (the fly). Located at 11h 41m 07.02s −65° 45′ 19.1″, it is a binary pair composed of a white dwarf
PSR_J1141−6545
Classification in astronomy
the first neutron star was not observed until 1967 when the first radio pulsar was discovered, neutron stars were proposed by Baade and Zwicky in 1933
Compact_object
Ancient circumbinary jovian exoplanet orbiting PSR B1620-26 binary system
period of the pulsar). In the early 1990s, a group of astronomers led by Donald Backer, who were studying what they thought was a binary pulsar, determined
PSR_B1620−26_b
Astrophysical phenomenon
at first, a puzzle. Some considered rotational energy from the central pulsar as a source. Although the energy that initially powers each type of supernovae
Supernova
X-ray binaries in the Large Magellanic Cloud
LMC X-4 is an eclipsing high-mass X-ray binary (HMXB) pulsar system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way approximately
LMC_X-4
Nebula powered by the pulsar wind of a pulsar
A pulsar wind nebula (PWN, plural PWNe), sometimes called a plerion (derived from the Greek "πλήρης", pleres, meaning "full"), is a type of nebula sometimes
Pulsar_wind_nebula
Theory of gravity by Albert Einstein
in 1974 in a binary pulsar called PSR1913+16. In such a system, one of the orbiting stars is a pulsar. This has two consequences: a pulsar is an extremely
Introduction to general relativity
Introduction_to_general_relativity
Device used to measure gravitational waves
wavelengths of a few thousand kilometers from a merging binary of stellar black holes. In June 2023, four pulsar timing array collaborations presented the first
Gravitational-wave observatory
Gravitational-wave_observatory
Hypothetical gravitational particle
to have been performed regarding this issue, it has been argued that binary pulsars should give greater constraints on the existence of the pressuron because
Pressuron
American astrophysicist
now scores of binary pulsars known, and independent measurements have confirmed Taylor's results. Taylor has used this first binary pulsar to make high-precision
Joseph_Hooton_Taylor_Jr.
Astronomy organization
Parkes Pulsar Timing Array in Australia, the European Pulsar Timing Array, and the Indian Pulsar Timing Array as part of the International Pulsar Timing
North American Nanohertz Observatory for Gravitational Waves
North_American_Nanohertz_Observatory_for_Gravitational_Waves
Intermediate-mass binary pulsar
PSR J2222−0137 is a nearby intermediate-mass binary pulsar at a distance of 267+1.2 −0.9 pc (approximately 870 light-years), whose low-mass neutron star's
PSR_J2222−0137
Radio telescope array
visible from its site, to search for transient sources. A secondary goal is pulsar timing, to aid in the search for gravitational waves. The project is managed
Deep_Synoptic_Array
Gravitational-wave event detected in 2023
the two LIGO detectors on 23 November 2023. As of 2025, it is the largest binary black hole merger yet detected, at 225+26 −43 solar masses (M☉) for the
GW231123
Gravitational-wave observation
Graham, M.J.; et al. (2020). "Candidate Electromagnetic Counterpart to the Binary Black Hole Merger Gravitational-Wave Event S190521g" (PDF). Physical Review
GW190521
Five-radio telescope collaboration to track stellar remnants' gravitational waves
European Pulsar Timing Array (EPTA) is a European collaboration to combine five 100-m class radio-telescopes to observe an array of pulsars with the specific
European_Pulsar_Timing_Array
Two interrelated physics theories by Albert Einstein
of gravity. (This has been observed in the orbit of Mercury and in binary pulsars). Light deflection: Rays of light bend in the presence of a gravitational
Theory_of_relativity
Former radio telescope in Puerto Rico, United States
first binary pulsar PSR B1913+16, an accomplishment for which they later received the Nobel Prize in Physics. In 1982, the first millisecond pulsar, PSR
Arecibo_Telescope
High mass X-ray binary star in the constellation Centaurus
PSR B1259−63 is a pulsar and member of an eclipsing binary star system with the blue O9.5Ve-class star SS 2883. The pair has an eccentric orbit that is
PSR_B1259−63
energy and angular momentum gradually, as illustrated by the binary pulsar PSR B1913+16. For binary black holes, the numerical solution of the two-body problem
Two-body problem in general relativity
Two-body_problem_in_general_relativity
Japanese underground gravitational wave detector
designed to eventually be able to observe gravitational wave signatures from binary neutron star mergers at a distance of up to ~150 Mpc. KAGRA is operated
Kamioka Gravitational Wave Detector
Kamioka_Gravitational_Wave_Detector
Theoretical physicist and astronomer
observations of pulsars, includes several effects predicted by S. Kopeikin that are important for measuring parameters of the binary pulsars, for testing
Sergei_Kopeikin
Change in wavelength of light
observed from Earth, its light is undergoing a blueshift. Components of a binary star system will be blueshifted when moving towards Earth When observing
Redshift
Binary pulsar system in the constellation Pegasus
SDSS J230641.47+244055.8 (abbreviated as SDSS J2306) is a binary star system composed of a pulsar-like white dwarf and a red dwarf, located in the constellation
SDSS_J230641.47+244055.8
November 2022, 267 pulsars had been discovered in 36 globular clusters of the Milky Way. Out of 267 pulsars, two millisecond binary pulsars are located in
NGC_6652
Type of computing cluster
The Borg, a 52-node Beowulf cluster used by the McGill University pulsar group to search for pulsations from binary pulsars
Beowulf_cluster
German-born theoretical physicist (1879–1955)
February 2016. Retrieved 6 July 2016. "Gravity investigated with a binary pulsar-Press Release: The 1993 Nobel Prize in Physics". Nobel Foundation. Archived
Albert_Einstein
Binary star system in the constellation Scorpius
AR Scorpii (AR Sco) is a binary star system that consists of a pulsar-like white dwarf and a red dwarf star. It is located close to the ecliptic plane
AR_Scorpii
Planet outside of the Solar System
System. The first confirmed detection of an exoplanet was in 1992 around a pulsar, and the first detection around a main-sequence star was in 1995. A different
Exoplanet
Gravitational wave observatory unit, india
Proposed: Atom interferometers Indirect detection B-modes of CMB Pulsar timing array Binary pulsar Theory General relativity Tests of general relativity Metric
Indian Initiative in Gravitational-wave Observations
Indian_Initiative_in_Gravitational-wave_Observations
Pulsar–white dwarf binary system in Scorpius constellation
PSR J1614–2230 is a pulsar in a binary system with a white dwarf in the constellation Scorpius. It was discovered in 2006 with the Parkes telescope in
PSR_J1614−2230
Cavity of hot gas blown from a star
launches in 2032 and 2033. Cosmic wind Planetary wind Colliding-wind binary Pulsar wind nebula Galactic superwind Superwind Castor, J.; McCray, R.; Weaver
Stellar-wind_bubble
Cosmic stream of charged particles
Stellar wind Solar wind Planetary wind Stellar-wind bubble Colliding-wind binary Pulsar wind nebula Superwind Shelton, Jim (July 27, 2015). "Dust pillars of
Cosmic_wind
Proposed theories of gravity
been shown to be inconsistent with observations of the Hulse–Taylor binary pulsar. Some of these theories lead to cosmic acceleration at late times and
Bimetric_gravity
Binary star with an X-ray pulsar in the constellation Centaurus
X-ray pulsar List of X-ray pulsars Tjemkes, S. A.; Zuiderwijk, E. J.; Van Paradijs, J. (1986). "Optical light curves of massive X-ray binaries". Astronomy
Centaurus_X-3
1974 Binary pulsars A binary pulsar is a pulsar with a binary companion, often another pulsar, white dwarf or neutron star. The first binary pulsar, PSR
Timeline of United States discoveries
Timeline_of_United_States_discoveries
Research facility in Western Australia
Proposed: Atom interferometers Indirect detection B-modes of CMB Pulsar timing array Binary pulsar Theory General relativity Tests of general relativity Metric
AIGO
Strong stellar winds of a galactic scale in size
Stellar wind Solar wind Planetary wind Stellar-wind bubble Colliding-wind binary Pulsar wind nebula Superwind Lehnert, Matthew D.; Heckman, Timothy M.; Weaver
Galactic_superwind
Chinese space program
LISA-Taiji network has the potential to detect more than twenty stellar binary black holes (sBBHs), for which the error in luminous distance measurement
Taiji_program
System of two stars orbiting each other
include the white dwarf-pulsar binary PSR B1620-26, the subgiant-red dwarf binary Gamma Cephei, and the white dwarf-red dwarf binary NN Serpentis, among others
Binary_star
Device used in gravitational wave observatories
Proposed: Atom interferometers Indirect detection B-modes of CMB Pulsar timing array Binary pulsar Theory General relativity Tests of general relativity Metric
Weber_bar
Hypothetical type of planet that contains more carbon than oxygen
Technology in Australia reported that the millisecond pulsar PSR J1719-1438 may have a binary companion star, PSR J1719−1438 b, that has been crushed
Carbon_planet
Proposed ground-based gravitational wave observatory
observations of compact binary coalescences with far greater precision, depth, and survey size. In particular, CE will be able to observe binary black hole (BBH)
Cosmic Explorer (gravitational wave observatory)
Cosmic_Explorer_(gravitational_wave_observatory)
Italian astrophysicist
gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays". Monthly Notices of the Royal Astronomical
Alberto_Vecchio
Computer program for pulsars
models. Pulsar Binary pulsar Recursive acronym "Tempo". "Tempo Reference Manual". G. Hobbs; R. Edwards; R. Manchester (2006). "TEMPO2, a new pulsar timing
Tempo_(astronomy)
International physics organization
The Binary Black Hole Grand Challenge Alliance (BBH Challenge Alliance) was a scientific collaboration of international physics institutes and research
Binary Black Hole Grand Challenge Alliance
Binary_Black_Hole_Grand_Challenge_Alliance
detection of gravitational waves was confirmed from observations of a binary pulsar, but by the end of the 1970s, Weber's work was considered spurious as
List of experimental errors and frauds in physics
List_of_experimental_errors_and_frauds_in_physics
American scientist and science communicator (1934–1996)
another follows familiar Newtonian gravity. Gravitational lenses and binary pulsar spin-downs reveal general relativity in the depths of space. We could
Carl_Sagan
2015 European Space Agency spacecraft
Proposed: Atom interferometers Indirect detection B-modes of CMB Pulsar timing array Binary pulsar Theory General relativity Tests of general relativity Metric
LISA_Pathfinder
Interferometer which uses the wave-like nature of atoms
Proposed: Atom interferometers Indirect detection B-modes of CMB Pulsar timing array Binary pulsar Theory General relativity Tests of general relativity Metric
Atom_interferometer
Proposed space-borne gravitational-wave observatory
about 100,000 km. The nominal source of the observatory is a white-dwarf binary RX J0806.3+1527 (also known as HM Cancri). This could serve as a good calibration
TianQin
International physics organization
Abbott, B.P.; et al. (2016). "Observation of Gravitational Waves from a Binary Black Hole Merger". Phys. Rev. Lett. 116 (6) 061102. arXiv:1602.03837. Bibcode:2016PhRvL
LIGO_Scientific_Collaboration
include radio pulsars and gamma-ray bursts. He is known for measurements of the masses of neutron stars and for the use of binary pulsars to test the theory
Stephen_E._Thorsett
Effect of general relativity
Lense–Thirring effect has been observed in a binary system that consists of a massive white dwarf and a pulsar. Frame-dragging may be illustrated most readily
Frame-dragging
7th episode of the 4th season of Star Trek: Voyager
takes the helm and sets Voyager on a course between the components of a binary pulsar at full speed. The lead alien fails to regain helm control and threatens
Scientific Method (Star Trek: Voyager)
Scientific_Method_(Star_Trek:_Voyager)
Proposed gravitational wave detector
Proposed: Atom interferometers Indirect detection B-modes of CMB Pulsar timing array Binary pulsar Theory General relativity Tests of general relativity Metric
Einstein_Telescope
BINARY PULSAR
BINARY PULSAR
Female
Hebrew
Variant spelling of Hebrew Bina, BINAH means "intelligence, wisdom."Â
Boy/Male
Indian
An intimate particle of the God of heaven
Male
English
English unisex form of Latin Hilarius and Hilaria, HILARY means "joyful; happy."Â Originally, this was strictly a masculine name.
Boy/Male
American, Australian, French, German, Greek, Latin, Polish, Swedish
Cheerful; Happy; Joyful; Similar to Hilary
Surname or Lastname
English (chiefly South Yorkshire)
English (chiefly South Yorkshire) : topographic name for someone who lived on land enclosed by a bend in a river, from Old English binnan ēa ‘within the river’, or a habitational name from places in Kent called Binney and Binny, which have this origin.Scottish : habitational name from Binney or Binniehill near Falkirk, named in Gaelic as Beinnach, from beinn ‘hill’ + the locative suffix -ach.
Boy/Male
Irish
An ancient Irish name whos meaning is lost in antiquety.
Girl/Female
Indian
Modesty
Girl/Female
Hindu
Shore, Musical instrument, Goddess of wealth
Girl/Female
English
Originally a diminutive used for names ending in -bina, like Albina, Columbina, and Robina, now...
Male
Scandinavian
Scandinavian form of Old Norse Einarr, EINAR means "lone warrior."
Female
English
English pet form of German Belinda, possibly BINDY means "bright serpent" or "bright linden tree."
Boy/Male
Indian, Punjabi, Sikh
Blessing
Boy/Male
Latin
Happy; Cheerful.
Female
Hebrew
(×‘Ö¼Ö´×™× Ö¸×”) Hebrew name BINA means "intelligence, wisdom."Â
Girl/Female
Indian
(the wife of Sage Kashyap)
Surname or Lastname
English
English : variant spelling of Vickery.
Female
Turkish
Turkish name PINAR means "spring."
Girl/Female
Hindu
Shore, Musical instrument, Goddess of wealth
Male
Hindi/Indian
(विनय) Hindi name VINAY means "leading asunder."
Male
Hindi/Indian
Variant spelling of Hindi Vijay, BIJAY means "victory."
BINARY PULSAR
BINARY PULSAR
Boy/Male
Indian, Punjabi, Sikh
Elixir of Truth
Male
English
Old English name BARTLEY means "Bart's (Bartholomew's) meadow."
Girl/Female
Australian, French
Of the Nobility; Noble
Biblical
proud; quarrelsome (applied to Egypt)
Boy/Male
Indian
Graceful, Elegant, Connoisseur
Male
Egyptian
, the last king of the IIIrd Egyptian dynasty.
Boy/Male
Hindu, Indian
Aim Winner
Girl/Female
Indian
Goddess Parvati
Boy/Male
Australian, Biblical, Greek, Hebrew
A Thousand; Learned
Boy/Male
Tamil
Sudamsh | ஸà¯à®¤à®¾à®®à¯à®·Â
Gold
BINARY PULSAR
BINARY PULSAR
BINARY PULSAR
BINARY PULSAR
BINARY PULSAR
a.
Containing ten; tenfold; proceeding by tens; as, the denary, or decimal, scale.
n.
That which is constituted of two figures, things, or parts; two; duality.
n.
See Finery.
n.
A binary compound of silicon, or one regarded as binary.
a.
lasting for one day; as, a diary fever.
a.
Compounded or consisting of two things or parts; characterized by two (things).
n.
A binary compound of zinc.
n.
A canary bird.
n.
A binary compound of hydrogen; a hydride.
a.
Of or pertaining to the Canary Islands; as, canary wine; canary birds.
a.
Of a pale yellowish color; as, Canary stone.
n.
A binary compound of selenium, or a compound regarded as binary; as, ethyl selenide.
v. i.
To perform the canary dance; to move nimbly; to caper.
n.
A binary compound of phosphorus.
n.
Wine made in the Canary Islands; sack.
a.
Relating or belonging to bile; conveying bile; as, biliary acids; biliary ducts.
n.
A pale yellow color, like that of a canary bird.
a.
Of or pertaining to the urine; as, the urinary bladder; urinary excretions.
n.
A register of daily events or transactions; a daily record; a journal; a blank book dated for the record of daily memoranda; as, a diary of the weather; a physician's diary.
n.
A binary compound of iodine, or one which may be regarded as binary; as, potassium iodide.