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6 relations: Accretion disk, K-type main-sequence star, Light curve, Main sequence, X-ray binary, X-ray transient.
Accretion disk
An accretion disk is a structure (often a circumstellar disk) formed by diffused material in orbital motion around a massive central body.
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K-type main-sequence star
A K-type main-sequence star (K V), also referred to as an orange dwarf or K dwarf, is a main-sequence (hydrogen-burning) star of spectral type K and luminosity class V. These stars are intermediate in size between red M-type main-sequence stars ("red dwarfs") and yellow G-type main-sequence stars.
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Light curve
In astronomy, a light curve is a graph of light intensity of a celestial object or region, as a function of time.
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Main sequence
In astronomy, the main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness.
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X-ray binary
X-ray binaries are a class of binary stars that are luminous in X-rays.
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X-ray transient
X-ray emission occurs from many celestial objects.
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V2293 Ophiuchi, X-ray nova Ophiuchi 1993.
