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Limits on the x-ray emission from several hyperluminous iras galaxies.
Hyperluminous Infrared galaxies (HLIRGs).
S5 0014+81 is a distant, compact, hyperluminous, broad-absorption line quasar or blazar located near the high declination region of the constellation Cepheus, near the North Equatorial Pole.
The Federation ship was a dark, twisted hulk of metal, shredded beyond recognition as a starship except for the telltale warp signature residue and other forms of radia- tion associated with hyperluminous travel.
Some of these neutron stars and black holes have nearby companion stars, and become powerful sources of X-rays as they pull matter off their companions (also known as ultra and hyperluminous X-ray sources).
In addition, Cepheus also has the hyperluminous quasar S5 0014+81, hosting an ultramassive black hole in its core at 40 billion solar masses, about 10,000 times more massive than the central black hole of the Milky Way, making it the most massive black hole known in the universe.