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This is a binary star in which one member is sucking matter from the other.
Many stars occur in binary systems (see binary star), in which the two partners orbit their mutual centre of mass.
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Supernova remnants are more powerful X-ray sources; the strongest sources known in the Milky Way Galaxy are certain binary stars in which one star is probably a black hole.
It has generally been presumed that the objects in this class are binary star systems in which mass transfer leads to nuclear fusion on the surface of a white dwarf1.
contact binary A binary star system in which both stars have expanded to fill their Roche lobes and the surfaces of the two stars merge.
It is a spectroscopic binary star, one in which the companion star is only known through analysis of the spectra.
Similarly, X-ray binaries are generally accepted to be binary star systems in which one of the two stars is a compact object accreting matter from its companion.
The black holes were orbiting each other, presumably because they were the remains of a binary star system in which both stars were massive and became black holes when they died.
It is a binary star in the constellation Canis Major.
Alternatively, it could have been a massive binary-star system in which one of the stars weighed between 60 and 80 solar masses and the other roughly 48 suns.
In the December issue of the journal Astronomy & Astrophysics, University of California, Berkeley, astronomers and an international team of colleagues report that they were able to resolve in visible light the two stars in the binary star system Capella, which orbit one another at about the distance of Venus from the sun and until now have been indistinguishable from Earth.
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