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Double stars that show a significant interaction between their components
An Interacting binary star is a type of binary star in which one or both of the component stars has filled or exceeded its Roche lobe, also known as a
Interacting_binary_star
Binary star system whose component stars are very close
hypergiant previously thought to be a contact binary. Interacting binary star KIC 9832227, a contact binary and a previous candidate for stellar merger
Contact_binary
System of two stars orbiting each other
A binary star or binary star system is a system of two stars that are gravitationally bound to and in orbit around each other. Binary stars are among
Binary_star
Jamaican astronomer
physical dynamics of interacting binary stars systems. However, her pioneering research in the tomography of interacting binary star systems and cataclysmic
Mercedes_Richards
Astronomical phenomenon
a much younger star. An example of a star system exhibiting stellar vampirism is HR 6819. Interacting binary star Dunham, Will (2022-03-02). "Stellar 'vampire'
Stellar_vampirism
Stellar core remnant
light star to burn through its fuel, so any observed He-core white dwarfs are expected to result from mass loss to a companion in an interacting binary star
White_dwarf
Binary star system in the constellation Draco
CX Draconis is an interacting binary star system in the northern constellation of Draco, abbreviated CX Dra. It has the designation HD 174237 in the Henry
CX_Draconis
Stream of ionized matter flowing away from a rotating astronomical object
of jets known anywhere in the sky Bipolar jets ejected from the interacting binary star KX Andromedae Disk wind slower wide-angle outflow, often occurring
Astrophysical_jet
Binary star system in the constellation Canis Major
R Canis Majoris is an eclipsing interacting binary star system in the constellation Canis Major. It varies from magnitude 5.7 to 6.34. The system is unusual
R_Canis_Majoris
System consisting of two black holes in close orbit around each other
black holes themselves, binary black hole systems are classified as either stellar-mass—involving remnants of high-mass binary star systems or formed by
Binary_black_hole
Planetary nebula in the constellation Cepheus
The morphological features of the nebula may be explained by an interacting binary star system with one of the pair passing through the asymptotic giant
NGC_7354
Small number of stars that orbit each other
comets). A star system of two stars is known as a binary star, binary star system or physical double star. Systems with four or more components are rare
Star_system
Star system in the constellation Sagittarius
S2CID 125853869. Polidan, R. S. (June 1988), "A new study of the interacting binary star V356 Sgr", ESA, A Decade of UV Astronomy with the IUE Satellite
V356_Sagittarii
Collapsed core of a massive star
been detected are pulsars or a part of a binary system. Neutron stars in a binary system with a main sequence star can pull in large amounts of gas from
Neutron_star
Process where a red giant star engulfs a planet
Contact binary Interacting binary star Neutron star merger Stellar collision Leary, Ashlyn R.; McSwain, M. Virginia (April 2025). "Dinner with a Star: Stellar
Stellar_engulfment
Constellation split into two non-contiguous parts
doi:10.1086/175883. Mennickent, R. E.; Kolaczkowski, Z. (2009). "Interacting Binary Star Environments and the W Ser - DPV - Algol Connection". The Interferometric
Serpens
X-ray source
the birth of a symbiotic X-ray binary, a "first" in the lifecycle of an interacting binary star, or a zombie neutron star brought back to life by its neighboring
IGR_J17329-2731
American Jesuit priest and astronomer (1933–2020)
studied the polarization produced in cataclysmic variable stars, or interacting binary star systems that give off sudden bursts of intense energy, and dust
George_Coyne
Binary system consisting of a white dwarf and a main sequence star or a brown dwarf
post-common-envelope binary (PCEB) or pre-cataclysmic variable is a binary system consisting of a white dwarf or hot subdwarf and a main-sequence star or a brown
Post-common-envelope_binary
Large self-illuminated object in space
Clocchiatti, Alejandro (2017). "Type Ib and IIb Supernova Progenitors in Interacting Binary Systems". The Astrophysical Journal. 840 (1): 10. arXiv:1701.02089
Star
Nova seen in 1939
brightness. This is an interacting binary star system consisting of a 1.04±0.06M☉ white dwarf primary star and a 0.87±0.06M☉ main sequence star with a stellar
BT_Monocerotis
Constellation in the northern celestial hemisphere
Dziban) is a binary star divisible in binoculars and small amateur telescopes, 72 light-years from Earth. The primary is a yellow-white star of magnitude
Draco_(constellation)
Type of stellar collision
of UVB radiation from the Sun. They could also interact with the atmosphere, yielding weakly-interacting muons. The flux density of these generated particles
Neutron_star_merger
Open cluster in the constellation Musca
red colour along with blue ultraviolet colour and it could be an interacting binary star. The turnoff point is at 2.6 ±0.1 M☉. The members show small dispersions
NGC_4815
Multiple star system in the constellation of Lyra
Lyrae A, is itself a triple star system, consisting of an eclipsing binary pair (Aa) and a single star (Ab). The binary pair's two components are designated
Beta_Lyrae
Galaxies with interacting gravitational fields
may also lead to other phenomena such as star formation and black hole activity. A giant galaxy interacting with its satellites is common. A satellite's
Interacting_galaxy
innovative method visualizes gas flows in interacting binary star systems, advancing research on Algol binaries and magnetic fields in stellar interactions
Science and technology in Jamaica
Science_and_technology_in_Jamaica
American video game company
2014, retrieved December 2, 2020 "Olé!". Saber Interactive. August 1, 2016. Retrieved April 18, 2020. "Binary Motion". Retrieved April 24, 2022. Morgan, Thomas
Saber_Interactive
Triple star system in the constellation Sagittarius
"Hubble Space Telescope Detection of Binary Companions Around Three WC9 Stars: WR 98a, WR 104, and WR 112". Interacting Winds from Massive Stars. ASP Conference
WR_104
Model for the accretion of a uniform gas by a massive body
interstellar medium by neutron stars and black holes, or wind mass transfer in binary star systems. It is named after Hermann Bondi, Fred Hoyle, and Raymond Lyttleton
Bondi–Hoyle–Lyttleton accretion
Bondi–Hoyle–Lyttleton_accretion
Neighborhoods retrieved 18 Aug, 2010 Ridpath, Ian. "Johann Bayer's southern star chart". Wild, J. P.; Radhakrishnan, V. (1995). "John Gatenby Bolton. 5 June
List_of_astronomers
Variable star in Monoceros
V723 Monocerotis is a binary star in the constellation Monoceros. It is an ellipsoidal variable about 1,500 light-years distant, too faint to be seen
V723_Monocerotis
Star in the constellation Centaurus
hypothesized the star to be a contact binary, sharing a common envelope of material with a smaller yellow supergiant and secondary star, the two orbiting
HR_5171
Substellar object
dwarf binaries have a higher companion-to-host ratio q = M B / M A {\displaystyle q=M_{B}/M_{A}} for lower mass binaries. Binaries with a M-type star as
Brown_dwarf
Eclipsing variable star in the constellation Perseus
paradox in the theory of stellar evolution: although components of a binary star form at the same time, and massive stars evolve much faster than the
Algol
1986 video game
space exploration, combat, and trading role-playing video game created by Binary Systems and published by Electronic Arts in 1986. Originally developed for
Starflight
Star in the constellation Pegasus
IK Pegasi (or HR 8210) is a binary star system in the constellation Pegasus. It is just luminous enough to be seen with the unaided eye, at a distance
IK_Pegasi
Binary star in the constellation Cepheus
is an eclipsing binary star system located in the constellation Cepheus. It is both a B[e] star and shell star. As a 5th magnitude star, it is visible
VV_Cephei
Variable star that brightens unpredictably
but it is understood that these flares are induced by a companion star in a binary system which causes the magnetic field to become tangled. Additionally
Flare_star
Zodiac constellation in the southern hemisphere
accompanied by a star of magnitude 9.2; α2 Capricorni is accompanied by a star of magnitude 11.0; this faint star is itself a binary star with two components
Capricornus
Heterogeneous class of stars with unusual spectra
of NaSt1 (WR 122): Equatorial Mass Loss and X-rays from an Interacting Wolf–Rayet Binary". Monthly Notices of the Royal Astronomical Society. 1502 (3):
Wolf–Rayet_star
Gravitational process studied in astronomy
astronomy. Star formation theory, as well as accounting for the formation of a single star, must also account for the statistics of binary stars and the
Star_formation
Star in constellation Taurus
estimated to be approximately 300 AU away from the southern binary, with the separation of the binary believed to be approximately 7 AU with an orbital period
T_Tauri
Star in the constellation Aries
35 Arietis (abbreviated 35 Ari) is a binary star in the northern constellation of Aries. 35 Arietis is the Flamsteed designation. It is approximately
35_Arietis
Eclipsing binary star
U Cephei is an eclipsing binary star discovered in 1880. It consists of a blue-white main sequence star of spectral type B7/8V that is eclipsed every two
U_Cephei
Constellation in the southern celestial hemisphere
first known visible star system with a black hole, QV Telescopii (HR 6819), however observations in 2022 indicated that this is a binary system of two main-sequence
Telescopium
Planetary nebula
"sh 2-78 Search". Mohery, M.; Ali, A.; Mindil, A.; Alghamdi, S.A. "Interacting planetary nebulae III: Verification and galactic population based on
Sh_2-78
High mass X-ray binary in the constellation of Cygnus
a binary system which is pulling in a stream of gas from an ordinary star companion. It is one of only two known HMXBs containing a Wolf–Rayet star. It
Cygnus_X-3
Constellation in the northern celestial hemisphere
et al. (September 2008), "First Resolved Images of the Eclipsing and Interacting Binary β Lyrae", The Astrophysical Journal, 684 (2): L95–L98, arXiv:0808
Lyra
Star in the constellation Grus
after interacting with Sagittarius A*, the supermassive black hole at the center of the galaxy. It is possible that it was originally part of a binary system
S5-HVS1
Binary star system in the constellation Vulpecula
Vulpeculae, is a binary star system 64.5 light-years (19.8 parsecs) away in the constellation of Vulpecula (the Fox). The primary star is suspected to
HD_189733
Aspect of relativity in physics
by intervening matter. Sources that can be studied this way include binary star systems composed of white dwarfs, neutron stars, and black holes; events
Gravitational_wave
2015 detection made by LIGO interferometers
inferred only indirectly, via their effect on the timing of pulsars in binary star systems. The waveform, detected by both LIGO observatories, matched the
First observation of gravitational waves
First_observation_of_gravitational_waves
Two continuous flows of gas from the poles of a star
; Degroote, P. (2015-06-12). "IRAS 19135+3937: an SRd variable as interacting binary surrounded by a circumbinary disc". Monthly Notices of the Royal Astronomical
Bipolar_outflow
Star whose brightness fluctuates, as seen from Earth
neutron star, or stellar mass black hole. A notable example of such a variable X-ray source is Cygnus X-1. DQ Herculis systems are interacting binaries in
Variable_star
Constellation straddling the celestial equator
a yellow star of magnitude 3.4 and the secondary is a blue star of magnitude 6.7. However, there are several dimmer double stars and binary stars in Hydra
Hydra_(constellation)
Star in the constellation Taurus
main-sequence star. Its mass is 2.6 times that of the Sun and its surface glows with an effective temperature of 10,300 K. It may be a binary star itself, as
Chi_Tauri
Variable star in the constellation Cepheus
VizieR. Harries, T. J.; Hilditch, R. W.; Hill, G. (April 1998). "Interacting OB star binaries: LZ Cep, SZ Cam and IU AUR". Monthly Notices of the Royal Astronomical
LZ_Cephei
Black hole formed by a collapsed star
galaxies. Stellar black holes in close binary systems are observable when the matter is transferred from a companion star to the black hole; the energy released
Stellar_black_hole
et al. (2022-07-01). "Eta Carinae: An evolving view of the central binary, its interacting winds and its foreground ejecta". The Astrophysical Journal. 933
List_of_most_massive_stars
Star at the centre of the Solar System
The Sun is the star located at the centre of the Solar System. It is a massive sphere of hot plasma, heated to incandescence by nuclear fusion reactions
Sun
Variable star in the constellation Ursa Major
a binary star system in the northern circumpolar constellation of Ursa Major. It is a variable star, with AN Ursae Majoris being the variable star designation
AN_Ursae_Majoris
Theoretical stellar remnant
white dwarf to cool to 5 K (−268.15 °C; −450.67 °F); however, if weakly interacting massive particles (WIMPs) exist, interactions with these particles may
Black_dwarf
Planet that is outside the Milky Way galaxy
burst-planet has a mass of around 2.87 M🜨. If it is proven to be caused by a interacting planet and a magnetar, this would make it the most distant individually
Extragalactic_planet
American actor (born 2001)
Danielle (October 29, 2018). ""Chilling Adventures of Sabrina" Star Lachlan Watson on Non-Binary Identity and Telling a Bit of Their Own Story Through Susie
Lachlan_Watson
Stellar system in the constellation Carina
(1 July 2022). "Eta Carinae: An evolving view of the central binary, its interacting winds and its foreground ejecta". The Astrophysical Journal. 933
Eta_Carinae
Astrophysical phenomenon
mixture of single massive stars and stripped-envelope stars from interacting binary systems. The continued lack of unambiguous detection of progenitors
Supernova
orbit binary star systems (and 39 orbit multiple star systems with three or more stars). Specifically, they orbit what are known as "wide" binary star systems
Physics_and_Star_Wars
Catalogue of peculiar galaxies produced by Halton Arp
10770, are interacting pairs of galaxies with tidal tails that look similar to spiral arms. Many of these spiral galaxies are probably interacting with the
Atlas_of_Peculiar_Galaxies
George Gatewood; et al. (2003). "An Astrometric Study of the Low-Mass Binary Star Ross 614" (PDF). The Astronomical Journal. 125 (3): 1530–1536. Bibcode:2003AJ
List_of_nearest_stars
Star in the constellation Centaurus
IAU Catalog of Star Names, retrieved 22 February 2025. van Rensbergen, W.; et al. (February 2006), "Evolution of interacting binaries with a B type primary
Zeta_Centauri
2005 video game
for that movie's levels. For instance, the alternate soundtrack for the "Binary Sunset" was used in the second Chapter of Episode III, while "The Battle
Lego Star Wars: The Video Game
Lego_Star_Wars:_The_Video_Game
Star in the constellation Camelopardalis
Svoboda, P.; Demircan, O. (April 2012). "Northern Binaries in the Evrena Project". From Interacting Binaries to Exoplanets: Essential Modeling Tools Proceedings
15_Camelopardalis
Variable star in the constellation Ara
M.; Nysewander, M. C. (2010). "Ultraviolet study of the active interacting binary star R Arae using archivalIUEdata". Monthly Notices of the Royal Astronomical
R_Arae
Spherical collection of stars
dynamical heating effect of binary star systems works to prevent an initial core collapse of the cluster. When a star passes near a binary system, the orbit of
Globular_cluster
Type of supernova in binary systems
occurs in binary systems (two stars orbiting one another) in which one of the stars is a white dwarf. The other star can be anything from a giant star to an
Type_Ia_supernova
Strong stellar winds of a galactic scale in size
charged particles, ejecta, and varying amounts of hot and cool gas, interacting with enough force that the ejecta's kinetic energy is converted to thermal
Galactic_superwind
Highly magnetic type of cataclysmic variable binary star system
highly magnetic type of cataclysmic variable (CV) binary star system, originally known as an AM Herculis star after the prototype member AM Herculis. Like
Polar_(star)
Fictional planets and moons in the Star Wars media franchise
The fictional universe of the Star Wars franchise features multiple planets and moons. While only the feature films and some other works are considered
List of Star Wars planets and moons
List_of_Star_Wars_planets_and_moons
Galaxy in the constellation Pavo
to be interacting with NGC 6872. Horrelou and Koribalski (2007), using a computer simulation to determine how the two galaxies were interacting, reported
NGC_6872
American science fiction television series
September 2020, non-binary newcomer Blu del Barrio was revealed to be portraying Adira, the first explicitly non-binary character within the Star Trek franchise
Star_Trek:_Discovery
Gamma-ray Binary in the Large Magellanic Cloud
LMC P3 (also known as 4FGL J0535.2-6736) is a gamma-ray binary star system located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky
LMC_P3
order to confirm the presence of the planet using the binary mass function. The speed of the star around the system's center of mass is much smaller than
Methods of detecting exoplanets
Methods_of_detecting_exoplanets
Triple star system in the constellation Scutum
though to be a detached eclipsing binary with additional irregular pulsations of the cool supergiant. Another star system similar to FR Scuti is TIC 290061484
FR_Scuti
Variable star in the constellation Serpens
doi:10.1086/175883. Mennickent, R. E.; Kolaczkowski, Z. (2009). "Interacting Binary Star Environments and the W Ser - DPV - Algol Connection". arXiv:0904
W_Serpentis
Variable star in the constellation Orion
FU Orionis is a variable and binary star system in the constellation of Orion, that in 1937 rose in apparent visual magnitude from 16.5 to 9.6, and has
FU_Orionis
Seyfert galaxy in the constellation Ursa Major
a velocity of −20,000 km s−1. The galaxy contains a curved radio jet interacting with the interstellar medium. Its position angle switches to −172° when
Markarian_231
Galactic X-ray source in the constellation Cygnus that is very likely a black hole
Cygnus X-1 is a high-mass X-ray binary system located about 7,000 light-years away, that includes a blue supergiant variable star. The supergiant and black
Cygnus_X-1
Star in the constellation Ursa Major
Majoris, as a representative of this type, may harbor two interacting processes: first, the star's strong magnetic field separating different elements in
Alioth
(1 July 2022). "Eta Carinae: an evolving view of the central binary, its interacting winds and its foreground ejecta". The Astrophysical Journal. 933
List_of_largest_stars
Variable star in the constellation Scorpius
from city lights. HD 159176 is the brightest star in the young open cluster NGC 6383. It is a binary star composed of two nearly identical O stars in a
HD_159176
Zhao; et al. (2008). "First Resolved Images Of The Eclipsing And Interacting Binary Beta Lyrae". The Astrophysical Journal. 684 (2): L95–L98. arXiv:0808
List of stars with resolved images
List_of_stars_with_resolved_images
Australian model (born 1995)
dance partner Lily Cornish after his father contracted COVID-19 after interacting with American actress Rita Wilson, who along with her husband Tom Hanks
Christian_Wilkins_(model)
Star in the constellation Centaurus
SV Centauri is a variable star in the constellation Centaurus. An eclipsing binary, its visual apparent magnitude has a maximum of 8.71, fading to 9.98
SV_Centauri
Star in the constellation Ursa Minor
RR Ursae Minoris, abbreviated RR UMi, is a binary star system in the northern circumpolar constellation of Ursa Minor. It can be viewed with the naked
RR_Ursae_Minoris
Star system in the constellation Boötes
CR Boötis is an interacting binary system in the northern constellation of Boötes, abbreviated CR Boo. It is one of the best-known AM Canum Venaticorum
CR_Boötis
Binary star with at least five exoplanets 41 light-years away
55 Cancri is a binary star system located 41 light-years away from the Sun in the zodiac constellation of Cancer. It has the Bayer designation Rho1 Cancri
55_Cancri
Fictional universe of a media franchise
planet located in the Outer Rim Territories of the galaxy, orbiting a binary star system. It is depicted as a remote, arid world with harsh climatic conditions
Universe_of_Star_Wars
1995 American science fiction television series
Star Trek: Voyager is an American science fiction series created by Rick Berman, Michael Piller and Jeri Taylor. It aired from January 16, 1995, to May
Star_Trek:_Voyager
Compact astronomical body
were consistent with a binary system of a massive star and compact star generating x-rays as gas from the massive but ordinary star was sucked into its invisible
Black_hole
INTERACTING BINARY-STAR
INTERACTING BINARY-STAR
Female
English
English pet form of German Belinda, possibly BINDY means "bright serpent" or "bright linden tree."
Boy/Male
Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Telugu
Good Looking; Interactive; Brightness
Male
Hindi/Indian
Variant spelling of Hindi Vijay, BIJAY means "victory."
Boy/Male
American, Australian, French, German, Greek, Latin, Polish, Swedish
Cheerful; Happy; Joyful; Similar to Hilary
Girl/Female
British, English, Hebrew
Interesting
Female
Turkish
Turkish name PINAR means "spring."
Boy/Male
Tamil
Interesting, Pleasant
Female
Hebrew
Variant spelling of Hebrew Bina, BINAH means "intelligence, wisdom."Â
Boy/Male
Hindu
Interesting, Pleasant
Male
Hindi/Indian
(विनय) Hindi name VINAY means "leading asunder."
Female
Hebrew
(×‘Ö¼Ö´×™× Ö¸×”) Hebrew name BINA means "intelligence, wisdom."Â
Male
Scandinavian
Scandinavian form of Old Norse Einarr, EINAR means "lone warrior."
Boy/Male
Hindu, Indian
Interesting
Boy/Male
Gujarati, Hindu, Indian, Kannada, Malayalam, Marathi, Telugu
Interesting
Boy/Male
Gujarati, Hindu, Indian, Kannada, Malayalam
Interesting; A Star
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.
Girl/Female
English
Originally a diminutive used for names ending in -bina, like Albina, Columbina, and Robina, now...
Girl/Female
Hindu, Indian
Interesting Person; Very Sweet
Male
English
English unisex form of Latin Hilarius and Hilaria, HILARY means "joyful; happy."Â Originally, this was strictly a masculine name.
Boy/Male
Indian, Punjabi, Sikh
Blessing
INTERACTING BINARY-STAR
INTERACTING BINARY-STAR
Boy/Male
British, English, Hungarian, Irish
Goshawk
Girl/Female
Hindu
Giving honor
Female
English
Anglicized form of Irish Gaelic Éirinn, ERIN means "Ireland."Â
Boy/Male
Gujarati, Hindu, Indian
Always Smiling; Joyful; Happy; Laughter; Laugh
Surname or Lastname
English and French
English and French : habitational name from the city of Arras in Artois, northern France, or one of the other places in France so named.Scottish : habitational name from Airhouse, a locality in Channelkirk, Berwickshire.English : habitational name from a place called Arras in East Yorkshire, earlier spelled Erghes, from the plural of Old Norse erg ‘hut’, ‘shelter’.German : metonymic occupational name for a cloth merchant, from a type of woolen cloth for which the city of Arras in Flanders was famous in the Middle Ages. This name is also established in Mexico.
Boy/Male
Bengali, Hindu, Indian, Kannada, Malayalam, Marathi, Telugu
Beloved of Lord Shree / Vishnu; Lover of Lakshmi
Boy/Male
Arabic, British, English, Jamaican
Adviser; Counsellor
Female
English
(الطير) Modern English unisex name derived from the name of the brightest star in the constellation Aquila, from an Arabic word ALTAIR means "the bird" or "the flyer."Â
Surname or Lastname
English
English : habitational name from a place called Ketton in Durham or one in Rutland or from Keaton in Ermington, Devon. The first is named from the Old English personal name Catta or the Old Norse personal name Káti + Old English tūn ‘settlement’; the second is probably from an old river name or tribal name Cētan (possibly a derivative of Celtic cēd ‘wood’) + Old English ēa ‘river’; and the last possibly from Cornish kee ‘hedge’, ‘bank’ + Old English tūn.
Boy/Male
English
Generous.
INTERACTING BINARY-STAR
INTERACTING BINARY-STAR
INTERACTING BINARY-STAR
INTERACTING BINARY-STAR
INTERACTING BINARY-STAR
v. i.
To perform the canary dance; to move nimbly; to caper.
a.
lasting for one day; as, a diary fever.
n.
Mutual or reciprocal action or influence; as, the interaction of the heart and lungs on each other.
a.
Of or pertaining to the Canary Islands; as, canary wine; canary birds.
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.
a.
Relating or belonging to bile; conveying bile; as, biliary acids; biliary ducts.
n.
A binary compound of silicon, or one regarded as binary.
n.
Wine made in the Canary Islands; sack.
n.
A binary compound of hydrogen; a hydride.
a.
Engaging the attention; exciting, or adapted to excite, interest, curiosity, or emotion; as, an interesting story; interesting news.
a.
Of a pale yellowish color; as, Canary stone.
a.
Containing ten; tenfold; proceeding by tens; as, the denary, or decimal, scale.
n.
A canary bird.
a.
Of or pertaining to the urine; as, the urinary bladder; urinary excretions.
n.
A pale yellow color, like that of a canary bird.
n.
A binary compound of selenium, or a compound regarded as binary; as, ethyl selenide.
n.
A binary compound of zinc.
n.
A binary compound of phosphorus.
n.
A binary compound of iodine, or one which may be regarded as binary; as, potassium iodide.
n.
See Finery.