Similarities between Astronomical object and Gamma-ray burst
Astronomical object and Gamma-ray burst have 30 things in common (in Unionpedia): Accretion disk, Binary star, Black hole, Blue supergiant star, Cambridge University Press, Comet, Earth, Elliptical galaxy, Galactic halo, Galaxy, Globular cluster, Interstellar medium, Luminous blue variable, Magnetar, Neutron star, Oxford University Press, Pulsar, Quark star, Quasar, Seyfert galaxy, Star, Stellar evolution, Sun, Superluminous supernova, Supermassive black hole, Supernova, Type Ib and Ic supernovae, Universe, White dwarf, Wolf–Rayet star.
Accretion disk
An accretion disk is a structure (often a circumstellar disk) formed by diffused material in orbital motion around a massive central body.
Accretion disk and Astronomical object · Accretion disk and Gamma-ray burst ·
Binary star
A binary star is a star system consisting of two stars orbiting around their common barycenter.
Astronomical object and Binary star · Binary star and Gamma-ray burst ·
Black hole
A black hole is a region of spacetime exhibiting such strong gravitational effects that nothing—not even particles and electromagnetic radiation such as light—can escape from inside it.
Astronomical object and Black hole · Black hole and Gamma-ray burst ·
Blue supergiant star
Blue supergiant stars are hot luminous stars, referred to scientifically as OB supergiants.
Astronomical object and Blue supergiant star · Blue supergiant star and Gamma-ray burst ·
Cambridge University Press
Cambridge University Press (CUP) is the publishing business of the University of Cambridge.
Astronomical object and Cambridge University Press · Cambridge University Press and Gamma-ray burst ·
Comet
A comet is an icy small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process called outgassing.
Astronomical object and Comet · Comet and Gamma-ray burst ·
Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life.
Astronomical object and Earth · Earth and Gamma-ray burst ·
Elliptical galaxy
An elliptical galaxy is a type of galaxy having an approximately ellipsoidal shape and a smooth, nearly featureless image.
Astronomical object and Elliptical galaxy · Elliptical galaxy and Gamma-ray burst ·
Galactic halo
A galactic halo is an extended, roughly spherical component of a galaxy which extends beyond the main, visible component.
Astronomical object and Galactic halo · Galactic halo and Gamma-ray burst ·
Galaxy
A galaxy is a gravitationally bound system of stars, stellar remnants, interstellar gas, dust, and dark matter.
Astronomical object and Galaxy · Galaxy and Gamma-ray burst ·
Globular cluster
A globular cluster is a spherical collection of stars that orbits a galactic core as a satellite.
Astronomical object and Globular cluster · Gamma-ray burst and Globular cluster ·
Interstellar medium
In astronomy, the interstellar medium (ISM) is the matter and radiation that exists in the space between the star systems in a galaxy.
Astronomical object and Interstellar medium · Gamma-ray burst and Interstellar medium ·
Luminous blue variable
Luminous blue variables (LBVs) are massive evolved stars that show unpredictable and sometimes dramatic variations in both their spectra and brightness.
Astronomical object and Luminous blue variable · Gamma-ray burst and Luminous blue variable ·
Magnetar
A magnetar is a type of neutron star with an extremely powerful inferred magnetic field (\sim 10^ - 10^ G).
Astronomical object and Magnetar · Gamma-ray burst and Magnetar ·
Neutron star
A neutron star is the collapsed core of a large star which before collapse had a total of between 10 and 29 solar masses.
Astronomical object and Neutron star · Gamma-ray burst and Neutron star ·
Oxford University Press
Oxford University Press (OUP) is the largest university press in the world, and the second oldest after Cambridge University Press.
Astronomical object and Oxford University Press · Gamma-ray burst and Oxford University Press ·
Pulsar
A pulsar (from pulse and -ar as in quasar) is a highly magnetized rotating neutron star or white dwarf that emits a beam of electromagnetic radiation.
Astronomical object and Pulsar · Gamma-ray burst and Pulsar ·
Quark star
A quark star is a hypothetical type of compact exotic star, where extremely high temperature and pressure has forced nuclear particles to form a continuous state of matter that consists primarily of free quarks, which can be modeled using the Calabi–Yau manifold.
Astronomical object and Quark star · Gamma-ray burst and Quark star ·
Quasar
A quasar (also known as a QSO or quasi-stellar object) is an extremely luminous active galactic nucleus (AGN).
Astronomical object and Quasar · Gamma-ray burst and Quasar ·
Seyfert galaxy
Seyfert galaxies are one of the two largest groups of active galaxies, along with quasars.
Astronomical object and Seyfert galaxy · Gamma-ray burst and Seyfert galaxy ·
Star
A star is type of astronomical object consisting of a luminous spheroid of plasma held together by its own gravity.
Astronomical object and Star · Gamma-ray burst and Star ·
Stellar evolution
Stellar evolution is the process by which a star changes over the course of time.
Astronomical object and Stellar evolution · Gamma-ray burst and Stellar evolution ·
Sun
The Sun is the star at the center of the Solar System.
Astronomical object and Sun · Gamma-ray burst and Sun ·
Superluminous supernova
A superluminous supernova (SLSN, plural superluminous supernovae or SLSNe; also known as hypernova) is a type of stellar explosion with a luminosity 10 or more times higher than that of standard supernovae.
Astronomical object and Superluminous supernova · Gamma-ray burst and Superluminous supernova ·
Supermassive black hole
A supermassive black hole (SMBH or SBH) is the largest type of black hole, on the order of hundreds of thousands to billions of solar masses, and is found in the centre of almost all currently known massive galaxies.
Astronomical object and Supermassive black hole · Gamma-ray burst and Supermassive black hole ·
Supernova
A supernova (plural: supernovae or supernovas, abbreviations: SN and SNe) is a transient astronomical event that occurs during the last stellar evolutionary stages of a star's life, either a massive star or a white dwarf, whose destruction is marked by one final, titanic explosion.
Astronomical object and Supernova · Gamma-ray burst and Supernova ·
Type Ib and Ic supernovae
Type Ib and Type Ic supernovae are categories of supernovae that are caused by the core collapse of massive stars.
Astronomical object and Type Ib and Ic supernovae · Gamma-ray burst and Type Ib and Ic supernovae ·
Universe
The Universe is all of space and time and their contents, including planets, stars, galaxies, and all other forms of matter and energy.
Astronomical object and Universe · Gamma-ray burst and Universe ·
White dwarf
A white dwarf, also called a degenerate dwarf, is a stellar core remnant composed mostly of electron-degenerate matter.
Astronomical object and White dwarf · Gamma-ray burst and White dwarf ·
Wolf–Rayet star
Wolf–Rayet stars, often abbreviated as WR stars, are a rare heterogeneous set of stars with unusual spectra showing prominent broad emission lines of highly ionised helium and nitrogen or carbon.
Astronomical object and Wolf–Rayet star · Gamma-ray burst and Wolf–Rayet star ·
The list above answers the following questions
- What Astronomical object and Gamma-ray burst have in common
- What are the similarities between Astronomical object and Gamma-ray burst
Astronomical object and Gamma-ray burst Comparison
Astronomical object has 260 relations, while Gamma-ray burst has 173. As they have in common 30, the Jaccard index is 6.93% = 30 / (260 + 173).
References
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