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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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
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
Bipolar planetary nebula in the constellation Hercules
Journal. 372: 215. doi:10.1086/169967. Livio, M.; Soker (May 1989). "Interacting winds and the shaping of planetary nebulae". The Astrophysical Journal
Humason_2-1
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
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
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
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
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
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
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)
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
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
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
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
Eclipsing binary in Scutum
RY Scuti is an eclipsing binary in the constellation of Scutum. It consists of a massive central star with an accretion disc and a blue supergiant donor
RY_Scuti
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
X-ray binary in Cygnus containing a stellar 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 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
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
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
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
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
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
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
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
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
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
Belgian astronomer
Day-Jones, A. C.; Koppen, J. (2012). "An Interacting Binary System Powers Precessing Outflows of an Evolved Star". Science. 338 (6108): 773–775. arXiv:1211
Henri_M._J._Boffin
X-ray binary system in the constellation Lacerta
MWC 656 is an X-ray binary star system in the northern constellation of Lacerta. It has the identifier HD 215227 from the Henry Draper Catalogue. With
MWC_656
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
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
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. Nine stars
Flare_star
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
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
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
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
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
Star in the constellation Libra
49 Librae is a binary star system in the Zodiac constellation of Libra. It has an apparent visual magnitude of 5.47, making it faintly visible to the
49_Librae
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
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
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
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 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
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
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)
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
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
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
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
Star in the constellation Ara
designation, V829 Arae, in 1987. The system appears to be a close, interacting binary with a hot secondary component of class A or hotter. It forms a suspected
HR_6384
Star in the constellation Lacerta
is a spectroscopic binary in the constellation Lacerta. Its apparent magnitude is 4.36. 5 Lacertae is a slow irregular variable star with a small amplitude
5_Lacertae
Type Ic supernova in the interacting galaxy NGC 4038
type WC Wolf-Rayet star with a mass over 40 times that of the Sun, or a star 20 to 40 times as massive as the Sun in a binary star system. Modjaz, M.;
SN_2004gt
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
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
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
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
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
Astrophysical phenomenon
mixture of single massive stars and stripped-envelope stars from interacting binary systems. The continued lack of unambiguous detection of progenitors
Supernova
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)
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
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
Binary star in the constellation Auriga
WW Aurigae is an eclipsing binary star system in the northern constellation of Auriga. It has a combined maximum apparent visual magnitude of 5.86, which
WW_Aurigae
American financial services firm
and Kalshi. The authority believes that event contracts are structured as binary options, long banned in Europe because of their gambling nature. In 2025
Interactive_Brokers
2000 video game
1990s, the British studio Binary Asylum – developer of Zeewolf – was approached by Interplay to develop a real-time strategy Star Trek game. First results
Star_Trek:_New_Worlds
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
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
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
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
Type of stellar binary
Variable (DPV) is a type of binary star. As the name implies, the systems vary in brightness not only due to eclipses of one star by the other, but also on
Double_periodic_variable
(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
Binary star in the constellation Scorpius
of the Sun. Antares appears as a single star when viewed with the naked eye, but it is actually a binary star system, with its two components called α
Antares
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
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
Planets and moons in the Star Wars media franchise
The Universe of the Star Wars franchise features multiple planets and moons. While only the feature films and some other works are considered canon to
List of Star Wars planets and moons
List_of_Star_Wars_planets_and_moons
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