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physical object > natural object > celestial body > collection of stars > collection of galaxies > galaxy cluster > Centaurus cluster |
Centaurus cluster comparison table |
Subject | has number of galaxie | is part of | is a kind of | has catalog | has wavelength | is an instance of | has synonym | has definition | has distance |
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galaxy cluster | 102 to 103 (order of magnitude) | collection of galaxies | catalog about star systems | An aggregate of galaxies. Bautz and Morgan divide them into three morphological types: type I contains a supergiant cD galaxy; Coma is type II, type III contains no members significantly brighter than the general bright population. Virgo is type III. 21 known X-ray sources are associated with clusters of galaxies. | |||||
X-ray source | celestial sphere | celestial body | X-ray | A class of celestial objects whose dominant mechanism of energy dissipation is through X-ray emission. Galactic X-ray sources appear optically as starlike objects, peculiar in their ultraviolet intensity, variability (on time scales ranging from milliseconds to weeks), and spectral features. All known compact X-ray sources are members of close binary systems; a current popular model is mass accretion onto a compact object from a massive companion. (Four X-ray sources - all variable - are known to be associated with globular clusters.) The 21 known extended X-ray sources associated with clusters of galaxies seem to be clouds of hot gas trapped in the cluster's gravitational field. | |||||
Centaurus cluster | 102 to 103 (order of magnitude) | celestial sphere | catalog about star systems | X-ray | X-ray source | 3U 1247-41 | A cluster of galaxies. Its radio counterpart is compact and located inside NGC 4696. | 200 Mpc |
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