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Binary star system in which two massive stars emit powerful stellar winds
A colliding-wind binary is a binary star system in which the two members are massive stars that emit powerful, radiatively-driven stellar winds. The location
Colliding-wind_binary
Flow of gas ejected from the upper atmosphere of a star
enough mass in their winds.[citation needed] Space portal Cosmic ray Cosmic wind Planetary wind Colliding-wind binary Pulsar wind nebula Galactic superwind
Stellar_wind
Model for the accretion of a uniform gas by a massive body
time-dependent medium. In colliding-wind binary systems, for example, the wind of the accreting star may oppose the incoming wind, while shocks, radiative
Bondi–Hoyle–Lyttleton accretion
Bondi–Hoyle–Lyttleton_accretion
Strong stellar winds of a galactic scale in size
intergalactic medium. Cosmic wind Stellar wind Solar wind Planetary wind Stellar-wind bubble Colliding-wind binary Pulsar wind nebula Superwind Lehnert,
Galactic_superwind
Triple-star system in the constellation Norma
idea that Apep was a new colliding-wind binary but the radio emission would make it the brightest radio colliding-wind binary discovered outside of the
Apep_(star_system)
Cavity of hot gas blown from a star
bubble, with launches in 2032 and 2033. Cosmic wind Planetary wind Colliding-wind binary Pulsar wind nebula Galactic superwind Superwind Castor, J.;
Stellar-wind_bubble
Nebula powered by the pulsar wind of a pulsar
Crab Nebula Cosmic wind Stellar wind Solar wind Planetary wind Stellar-wind bubble Colliding-wind binary Galactic superwind Superwind Orders of magnitude
Pulsar_wind_nebula
Star in the constellation of Cygnus
its episodic dust formation. It is now regarded as the prototype colliding-wind binary. Shortly after periastron passage every eight years, the infrared
WR_140
Stars sorted by absolute magnitude
"On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary". The Astrophysical
List_of_most_luminous_stars
"On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary". The Astrophysical
List_of_most_massive_stars
Dense stellar wind
wind envelope becomes its planetary nebula. Cosmic wind Solar wind Stellar wind Planetary wind Stellar-wind bubble Colliding-wind binary Pulsar wind nebula
Superwind
Open cluster in the constellation of Serpens
over-contact eclipsing binary MY Ser. It is one of the most luminous stars in the galaxy. HD 168112 is another colliding-wind binary in the cluster; both
NGC_6604
Heterogeneous class of stars with unusual spectra
Bolingbroke, N.J. (2005). "High-resolution radio observations of the colliding-wind binary WR 140". The Astrophysical Journal. 623 (1): 447–459. arXiv:astro-ph/0501391
Wolf–Rayet_star
Cosmic stream of charged particles
weight. Galactic superwind Stellar wind Solar wind Planetary wind Stellar-wind bubble Colliding-wind binary Pulsar wind nebula Superwind Shelton, Jim (July
Cosmic_wind
Star system in the constellation Vela
category of Particle-Accelerating Colliding-Wind Binaries (PACWB), binary systems made of massive stars whose winds collide, resulting in particle acceleration
Gamma_Velorum
Wolf–Rayet star in the constellation Dorado
R136a1/2 showed relatively soft x-rays not thought to indicate a colliding winds binary. Rapid Doppler radial velocity variations would be expected from
R136a1
Triple star system in the constellation Carina
(2016). "A model for the non-thermal emission of the very massive colliding-wind binary HD 93129A". Astronomy & Astrophysics. 591: A139. arXiv:1604.07294
HD_93129
Star in the constellation Virgo
G. Jr.; Penny, Laura R. (April 1997). "Photospheric Heating in Colliding-Wind Binaries". Astrophysical Journal. 479 (1): 408. Bibcode:1997ApJ...479..408G
Spica
Open cluster in the constellation Scorpius
a colliding-wind binary, based on data from XMM-Newton. In contrast, WR 87 has a high plasma temperature consistent with that of a colliding-wind binary
HM_1
Triple star system in the constellation Sagittarius
ISSN 0035-8711. Hill, G M (October 4, 2024). "Is WR 104 a face-on, colliding-wind binary?". Monthly Notices of the Royal Astronomical Society. 534 (3): 2184–2195
WR_104
Star system in the constellation of Cygnus
leading to a separation of about 0.33 AU. WR 140, the prototype colliding-wind binary Roman, Nancy G. (1987). "Identification of a constellation from
WR_147
Super star cluster in the Milky Way Galaxy
infra-red emission) that are typical of colliding-wind binaries or dust-forming Wolf–Rayet stars. Overall binary fractions of 70% for the Wolf–Rayet population
Westerlund_1
Blue hypergiant star
"On the Binary Nature of Massive Blue Hypergiants: High-resolution X-Ray Spectroscopy Suggests That Cyg OB2 12 is a Colliding Wind Binary". The Astrophysical
Cygnus_OB2-12
Binary star system in the constellation Carina
Solivella, G. (2006). "The first orbital solution for the massive colliding-wind binary HD 93162 (≡WR 25)". Astronomy and Astrophysics. 460 (3): 777–782
WR_25
Binary star in the constellation Carina
"O". WR 30a is a very strong x-ray source. This is expected for a colliding-wind binary, but the source of the x-rays has not been conclusively determined
WR_30a
Stellar system in the constellation Carina
the X-ray emission presumed to originate in a colliding wind zone. The confirmation of a luminous binary companion greatly modified the understanding of
Eta_Carinae
Collapsed core of a massive star
stars that have 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
Neutron_star
Wolf-Rayet star and spectroscopic binary star in the constellation of Cygnus
M.; Schanne, L.; et al. (2011). "Spectroscopy of the archetype colliding-wind binary WR 140 during the 2009 January periastron passage". Monthly Notices
WR_133
Binary star in the Large Magellanic cloud
known binary system. Melnick 34 is a binary star with an orbital period of 155 days. It shows high x-ray luminosity characteristic of colliding-wind binaries
Melnick_34
Cluster of massive and luminous stars
R.; Van Loo, S. (2006). "XMM-Newton observations of the massive colliding wind binary and non-thermal radio emitter CygOB2#8A [O6If + O5.5III(f)]" (PDF)
Cygnus_OB2
Star in the constellation Triangulum Australe
binary (WC9d + O) star, with a period of 2.293 days and an amplitude of 0.044 magnitudes, suggesting it could be a short period colliding-wind binary
WR_69
List from the Alphabet Direction (αβ)
(planetary nebulae) PACWB — Catalogue of Particle-Accelerating Colliding-Wind Binaries [7] Pe — Perek (planetary nebulae) Perr — Perrotin (double stars)
List of astronomical catalogues
List_of_astronomical_catalogues
Effect in spectroscopy
line strengths. Colliding-wind binary Palate, M.; Rauw, G.; Koenigsberger, G.; Moreno, E. (2013). "Spectral modelling of massive binary systems". Astronomy
Struve–Sahade_effect
Spectroscopic binary star near the center of Cygnus OB2
R.; Van Loo, S. (2006). "XMM-Newton observations of the massive colliding wind binary and non-thermal radio emitter CygOB2#8A [O6If + O5.5III(f)]" (PDF)
Cygnus_OB2-8A
Binary star located in the Small Magellanic Cloud in the constellation Hydrus
stars are expected to produce copious x-ray emission from colliding winds. The colliding winds are detected via their impact on emission lines in the spectrum
AB8_(star)
Star in the constellation Dorado
binary, due to the detection of hard x-ray emission typical of colliding wind binaries, but the companion is thought to make only a small contribution
R136c
Binary Star in the Cygnus OB2 association
observed in optical spectroscopy. The colliding stellar winds produce thermal X-ray emission from shocks in the wind-wind collision region (WWCR), with luminosities
Cygnus_OB2-9
Binary star in the constellation Carina
C. A.; Cohen, D. H.; Owocki, S. P. (2012). "An X-Ray Survey of Colliding Wind Binaries". Proceedings of a Scientific Meeting in Honor of Anthony F. J
WR_22
Galactic X-ray source in the constellation Cygnus that is very likely a black hole
X-ray bursts lasting only for about 1 ms. Cygnus X-1 is a high-mass X-ray binary system located about 7,000 light-years away, that includes a blue supergiant
Cygnus_X-1
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
Meteorological phenomenon involving two cyclones circling each other
Fujiwhara effect, sometimes referred to as the Fujiwhara interaction or binary interaction, is a phenomenon that occurs when two nearby cyclonic vortices
Fujiwhara_effect
Aftermath of a neutron star merger
event that occurs in a compact binary system when two neutron stars (BNS) or a neutron star and a black hole collide. The kilonova, visible over the
Kilonova
Spectroscopic binary star in the constellation Monoceros
hours, thought to be due to many factors including the binary orbit, hot spots in the colliding winds, and granulation. The luminosities of each component
Plaskett's_Star
Coming together of two stars
by stellar dynamics within a star cluster, or by the orbital decay of a binary star due to stellar mass loss or gravitational radiation, or by other mechanisms
Stellar_collision
Star in the constellation Musca
J.; St-Louis, N. (1 October 2002). "Modelling the colliding-winds spectra of the 19-d WR + OB binary in the massive triple system Muscae". Monthly Notices
Theta_Muscae
Star in the constellation Carina
Naze, Yael (2016). "The X-ray light curve of the massive colliding wind Wolf-Rayet + O binary WR21a". Astronomy & Astrophysics. 1604: A113. arXiv:1604
WR_21a
Stellar core remnant
dwarf is Sirius B, at 8.6 light years, the smaller component of the Sirius binary star. In 1910, Henry Norris Russell, Edward Charles Pickering and Williamina
White_dwarf
American drama television series by Taylor Sheridan and Christian Wallace
platform in the Gulf Bobbi Salvör Menuez as Paigyn Meester, Ainsley's non-binary almost roommate at TCU Mackenzie Astin as Detective Hayes, Odessa Police
Landman_(TV_series)
Triple star system in the constellation Tucana
Luminous Eclipsing SMC OB + WN Binary HD 5980 before and during the Recent LBV-like Outburst: An Extreme Case of Colliding Winds". The Astrophysical Journal
HD_5980
Star in the constellation Crux
S2CID 10513657. Zhekov, S. A. (2012). "X-rays from colliding stellar winds: The case of close Wolf-Rayet+O binary systems". Monthly Notices of the Royal Astronomical
WR_46
American astronomer, scientist, and science communicator
measurement of binary stars, receiving a bachelor's degree in 1992. At Georgia State University Thaller worked on colliding winds in close massive binary systems
Michelle_Thaller
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
First observation of gravitational waves
First_observation_of_gravitational_waves
Variable star in the constellation Scorpius
Wiemker, R. (June 2001). "A Spectroscopic Search for Colliding Stellar Winds in O-Type Close Binary Systems. V. HD 149404". The Astrophysical Journal. 554
HD_149404
Substellar object
by winds on the brown dwarfs. Additionally, absorption signatures of carbon monoxide, methane, and water vapor were detected. Brown dwarfs binaries of
Brown_dwarf
Binary star in the constellation Aries
BD+20°307 is a close binary star system approximately 300 light-years away in the constellation Aries. The system is surrounded by a dusty ring, and probably
BD+20°307
Star in the constellation of Scorpius
Becker, M.; Raucq, F. (2013). "Catalogue of particle-accelerating colliding-wind binaries". Astronomy & Astrophysics. 558: A28. arXiv:1308.3149. Bibcode:2013A&A
HD_151932
Astrophysical phenomenon
Danchi, W. C.; Owocki, S. P.; Gayley, K. G. (2008). "The Prototype Colliding-Wind Pinwheel WR 104". The Astrophysical Journal. 675 (1): 698–710. arXiv:0712
Supernova
Diffuse nebula in the constellation Orion
when two particle streams collide with each other. They are present near the hottest stars in the nebula where the stellar wind speed is estimated to be
Orion_Nebula
Binary star in the Small Magellanic Cloud in the constellation Tucana
WR/O binary, due to colliding winds being shocked to extreme temperatures. The x-ray luminosity varies during the orbit. Although the stellar winds of WR
AB7
Hypothetical hybrid star type
object would be formed when a neutron star collides with another star, often a red giant or supergiant. The colliding objects can simply be wandering stars
Thorne–Żytkow_object
Galaxy merger remnant in the constellation Ophiuchus
scientists have concluded that this galaxy has reached its last stages before colliding into one another. Photographic evidence proves that the two nuclei have
NGC_6240
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
Binary star in the constellation of Cygnus
little doubt that it is a binary system, due to the regular variations and the presence of hard x-ray radiation from colliding winds, but the secondary is
WR_148
Australian astronomer
revealed pinwheel nebulae around Wolf–Rayet stars, formed by winds colliding with their binary companions. The most spectacular of these have been conjectured
Peter_Tuthill_(astronomer)
Binary star system in the constellation Carina
the individual components varies during the orbit. It also has colliding stellar winds that produce variable x-ray and non-thermal radio emission. List
HD_93403
Binary star system
F. J.; St-Louis, N. (March 2018), "Modelling the colliding-wind spectra of the WC8d+O8-9IV binary CV Ser (WR 113)", Monthly Notices of the Royal Astronomical
CV_Serpentis
Matter and radiation in the space between the star systems in a galaxy
in interstellar space came in 1904, when Johannes Hartmann observed the binary star Mintaka (Delta Orionis) with the Potsdam Great Refractor. Hartmann
Interstellar_medium
Compact astronomical body
hole, this shadow is the limit for possible observations. The shadow of colliding black holes should have characteristic warped shapes, allowing scientists
Black_hole
Binary star in the constellation Cygnus
X-ray binaries with accreting companions. When combined with the unique spectral features, this suggested an orbiting collapsed star was colliding with
HD_191612
European space mission to measure gravitational waves
known as extreme mass ratio inspirals, binaries of compact stars, substellar objects orbiting such binaries, and possibly other sources of cosmological
Laser Interferometer Space Antenna
Laser_Interferometer_Space_Antenna
Binary star system in the constellation Cepheus
of neutral hydrogen. A bow shock is being formed where the stellar wind is colliding with the surrounding interstellar medium. The peculiar velocity of
Delta_Cephei
Gravitational wave observatory site
such as gravitational waves caused by oscillating cosmic strings or colliding domain walls. LIGO operates two gravitational wave observatories in unison:
LIGO
Planetary nebula in the constellation Draco
possibly indicating a high frequency of binary companions to CSPNe. Other potential explanations include self-shocking winds or PN mass fallback." Planetary nebulae
Cat's_Eye_Nebula
Argentine astrophysicist
AGNs Accretion vs. colliding wind models for the gamma-ray binary LS I+ 61 303: an assessment Gamma-ray emission from Wolf-Rayet binaries Reissner-Nordström
Gustavo_E._Romero
Gravitational process studied in astronomy
the formation of a single star, must also account for the statistics of binary stars and the initial mass function. Most stars do not form in isolation
Star_formation
Branch of astronomy that uses X-ray observation
controversial with models including unstable stellar winds, colliding winds, magnetic coronae, disk coronae, wind-fed magnetospheres, accretion shocks, the operation
X-ray_astronomy
Scientific projections regarding the far future
Lawrance, Nicholas; Danchi, William; et al. (2008). "The Prototype Colliding-Wind Pinwheel WR 104". The Astrophysical Journal. 675 (1): 698–710. arXiv:0712
Timeline_of_the_far_future
Star in the constellation Carina
Cherepashchuk, A. M. (2025-10-19). "The massive binary system WR 20a: light curve analysis in a colliding wind model". arXiv:2510.16902 [astro-ph.SR]. Rauw;
WR_20a
Planets found orbiting pulsars
Ryosuke; Podsiadlowski, Philipp (2 November 2022). "neutron stars colliding with binary companions: formation of hypervelocity stars, pulsar planets, bumpy
Pulsar_planet
Class of X-ray binary stars
X-ray bursters are one class of X-ray binary stars exhibiting X-ray bursts, periodic and rapid increases in luminosity (typically a factor of 10 or greater)
X-ray_burster
Fictional eco-goth rock band
HBO Max series Velma. Thorn appears in season 2 as an adult who has a non-binary goth child named Amber. On August 26, 2025, "The Hex Girls: A Rogue Thorn
The_Hex_Girls
Shock wave caused by blowing stellar wind
stellar wind. Bow shock occurs when the magnetosphere of an astrophysical object interacts with the nearby flowing ambient plasma such as the solar wind. For
Bow_shock
Temperate gas giant in Kepler-47 system
Object of Interest designation KOI-3154.02) is an exoplanet orbiting the binary star system Kepler-47, the outermost of three such planets discovered by
Kepler-47c
Astronomical object
formed from the dust that is spewed out of a binary star system. The stellar winds of the two stars collide and form two dust lanes that spiral outward
Pinwheel_nebula
Binary star system in the constellation Cepheus
pair are a source of X-ray emission, which may be the result of colliding stellar winds. Their measured X-ray luminosity is 3.2×1031 erg s−1. The location
DH_Cephei
Binary star system in the constellation Carina
that MTT 68 is a binary due to its high x-ray luminosity, the observed companion is too distant to create the x-rays by colliding winds and a third, closer
MTT_68
Gravitational-wave detector in Italy
short period. The main sources in this category are compact binary coalescences (CBC) from binary black holes (or neutron stars) merging, emitting a rapidly-growing
Virgo_interferometer
1887 investigation of the speed of light
including their laboratory, through the luminiferous aether, or "aether wind" as it was sometimes called. The result was negative, in that Michelson and
Michelson–Morley_experiment
Star system in the constellation Carina
days. The system is bright at x-ray wavelengths primarily due to colliding stellar winds in the two close pairs. Pair A1/A2 contributes the bulk of the
QZ_Carinae
Star in the constellation Vela
WR+O Binaries". Astronomical Journal. 112: 2227. Bibcode:1996AJ....112.2227L. doi:10.1086/118175. Fahed, R.; Moffat, A. F. J. (2012). "Colliding winds in
WR_12
Bright massive star system
radiation from the vicinity of Pismis 24-1 is assumed to be caused by the colliding winds of these two supergiants. Pismis 24-1SW is apparently a single star
Pismis_24-1
Constellation split into two non-contiguous parts
from Earth. It consists of two large spiral galaxies in the process of colliding with their nuclei orbiting at a distance of 1,200 light-years, causing
Serpens
Small patches of nebulosity associated with newly born stars
high-speed collisions. This suggests that some of the material they are colliding with is also moving along the beam, although at a lower speed. Spectroscopic
Herbig–Haro_object
and takes it back with him to his reality. B.A.R.F., which stands for Binarily Augmented Retro-Framing, is a holographic technology created by Quentin
Features of the Marvel Cinematic Universe
Features_of_the_Marvel_Cinematic_Universe
American television series
Ana, who is also Ana's right-hand. The character was reimagined as non-binary for the show. Ira Munn and Lucy Currey as Punch and Judy: The duo hosts
Cowboy_Bebop_(2021_TV_series)
Season of television series
del Sur, due to Teeny Chirichillo participating in Survivor 47 as a non-binary person. Chirichillo would come out as a transgender man in April 2025. At
Survivor_47
Star not gravitationally bound to any galaxy
like other stars, before being expelled as the result of either galaxies colliding or of a multiple-star system traveling too close to a supermassive black
Intergalactic_star
Constellation in the northern celestial hemisphere
per second). Its magnetic field and wind of particles creates a visible bow shock 4 light-years ahead of it, colliding with the diffuse, and usually invisible
Cassiopeia_(constellation)
Largest dwarf planet
the Sun than Neptune, but a stable orbital resonance prevents them from colliding. Pluto has five known moons: Charon, the largest, whose diameter is just
Pluto
Device used to measure gravitational waves
gravitational waves with wavelengths of a few thousand kilometers from a merging binary of stellar black holes. In June 2023, four pulsar timing array collaborations
Gravitational-wave observatory
Gravitational-wave_observatory
COLLIDING WIND-BINARY
COLLIDING WIND-BINARY
Boy/Male
Welsh English
Handsome.
Surname or Lastname
English
English : topographic name for someone who lived near a pathway, alleyway, or road, Old English (ge)wind (from windan ‘to go’).English, German, and Danish : nickname for a swift runner, from Middle English wind ‘wind’, Middle High German wint ‘wind’, also ‘greyhound’.German : variant of Wendt.Swedish : ornamental name from vind ‘wind’, or a habitational name from a place named with this element.
Surname or Lastname
English
English : variant of Wynn.Americanized spelling of German Wein.
Surname or Lastname
English
English : variant of Winch.
Surname or Lastname
Danish
Danish : probably a habitational name from Kolding. This was originally the name of a river, from kaldr ‘cold’ + a derivational suffix -ung, hence ‘the cold river’.English : perhaps a spelling variant of Golding.
Girl/Female
Bengali, Indian
Kind; Find
Surname or Lastname
English
English : from Middle English wild ‘wild’, ‘uncontrolled’ (Old English wilde), hence a nickname for a man of violent and undisciplined character, or a topographic name for someone who lived on a patch of overgrown uncultivated land.English : habitational name from a place named Wyld, as for example in Berkshire and Dorset, both named from Old English wil ‘trap’, ‘snare’.German and Jewish (Ashkenazic) : cognate of 1, from Middle High German wilde, wilt, German wild ‘wild’, also used in the sense ‘strange’, ‘foreign’, and therefore in some cases a nickname for an incomer.
Surname or Lastname
English (central and northern)
English (central and northern) : nickname for a gentle or timid person, from Middle English, Old English hind ‘female deer’.English and Scottish : variant of Hine ‘servant’, with excrescent -d.
Surname or Lastname
English
English : from the Old Norse personal name Kollungr, a derivative of Koli, or from an Old English cognate, Colling, a derivative of Cola (see Cole 2).English : from a pet form of Coll 1.Altered spelling of German Kölling (see Kolling).
Boy/Male
Scandinavian
From the Island of the Wends (the Wends were an ancient Scandinavian tribe).
Surname or Lastname
German and Jewish (Ashkenazic)
German and Jewish (Ashkenazic) : from Middle High German kint, German Kind ‘child’, hence a nickname for someone with a childish or naive disposition, or an epithet used to distinguish between a father and his son. In some cases it may be a short form of any of various names ending in -kind, a patronymic ending of Jewish surnames.Dutch : variant spelling of Kint, cognate with 1, also found in such forms as ’t Kind and compounds such as Jongkind.English : nickname from Middle English kind (Old English gecynde) in any of its many senses: ‘legitimate’, ‘dutiful’, ‘benevolent’, ‘loving’, ‘gracious’.
Girl/Female
German
Snake.
Surname or Lastname
English
English : habitational name from places named Wing in Buckinghamshire and Rutland. The former was probably named in Old English as the settlement of the Wiwingas ‘the family or followers of a man named Wiwa’, or alternatively perhaps ‘the people of the temple’ (from a derivative of Old English wīg, wēoh ‘(pre-Christian) temple’). The latter is from Old Norse vengi, a derivative of vangr ‘field’. Compare Wang.Dutch (van Wing) : variant of Winge.Chinese : variant of Rong 2.
Boy/Male
Hindu, Indian, Traditional
Wild Wind
Girl/Female
Norse
A giant.
Girl/Female
Indian
India, Female deer
Surname or Lastname
English
English : perhaps a nickname for a shy or short-sighted person, from Old English wand ‘mole’. Compare Want.German : occupational name for a weaver or cloth cutter, from a reduced form of Middle High German gewant ‘cloth’, ‘garment’. Compare Wander 2.German : topographic name from Middle High German want ‘wall’, ‘steep rock’, ‘precipice’.Dutch : metonymic occupational name for a glove maker, from Middle Dutch wante ‘glove’.
Surname or Lastname
English
English : variant spelling of Wynn.Variant of Welsh Gwynn.
Male
English
Short form of English Winfred and Winifred, both WIN means "holy reconciliation," and other names beginning with Win-.Â
Girl/Female
American, Australian, Jamaican
Full of Wind; Windy; Blustery; Breezy
COLLIDING WIND-BINARY
COLLIDING WIND-BINARY
Boy/Male
Indian, Marathi
Joyful
Male
Japanese
(勇) Japanese name ISAMU means "courage."
Female
Scandinavian
Scandinavian form of Old Norse Ingrið, INGRID means "Ing-beautiful."
Girl/Female
Indian
Girl/Female
Indian, Kannada
Worshiper
Girl/Female
Gujarati, Hindu, Indian
Emotion
Girl/Female
Tamil
Rain
Girl/Female
Tamil
Sri Sai | à®·à¯à®°à¯€ ஸாஇ
Sai
Girl/Female
Indian
One without An end
Boy/Male
British, Christian, English, Scottish
Forsaken
COLLIDING WIND-BINARY
COLLIDING WIND-BINARY
COLLIDING WIND-BINARY
COLLIDING WIND-BINARY
COLLIDING WIND-BINARY
n.
A direction from which the wind may blow; a point of the compass; especially, one of the cardinal points, which are often called the four winds.
v. t.
To cover or surround with something coiled about; as, to wind a rope with twine.
v. t.
To expose to the wind; to winnow; to ventilate.
superl.
Next the wind; windward.
n.
Air or gas generated in the stomach or bowels; flatulence; as, to be troubled with wind.
a.
Anemophilous; fertilized by pollen borne by the wind.
superl.
Serving to occasion wind or gas in the intestines; flatulent; as, windy food.
v. t.
To drive hard, or force to violent exertion, as a horse, so as to render scant of wind; to put out of breath.
v. i.
To turn completely or repeatedly; to become coiled about anything; to assume a convolved or spiral form; as, vines wind round a pole.
a.
Having the taste or qualities of wine; vinous; as, grapes of a winy taste.
superl.
Exposed to the wind and sea; unsheltered; as, a wild roadstead.
a.
Colliding; clashing.
n.
Air artificially put in motion by any force or action; as, the wind of a cannon ball; the wind of a bellows.
superl.
Attended or caused by wind, or gas, in the intestines.
superl.
Consisting of wind; accompanied or characterized by wind; exposed to wind.
n.
A liquor or beverage prepared from the juice of any fruit or plant by a process similar to that for grape wine; as, currant wine; gooseberry wine; palm wine.
n.
A horse given to wind-sucking
v. i.
To have a circular course or direction; to crook; to bend; to meander; as, to wind in and out among trees.
a.
Windy; generating wind.
v.
Memory; remembrance; recollection; as, to have or keep in mind, to call to mind, to put in mind, etc.