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List of black holes

This list of black holes is organized by mass ; some items in this list are galaxies or star clusters that are believed to be organized around a black hole. Messier and New General Catalogue designations are given where possible.

Supermassive black holes and candidates
Ansky, a black hole in the SDSS1335+0728 galaxy • 1ES 2344+514Ton 618 (this quasar has possibly the biggest black hole ever found, estimated at 66 billion solar masses) • 3C 3714C +37.11 (this radio galaxy is believed to have binary supermassive black holes) • AP LibS5 0014+81 (said to be a compact hyperluminous quasar, estimated at 40 billion solar masses) • APM 08279+5255 (contains one of the largest black holes, estimated at 10-23 billion solar masses; previous candidate for largest) • Arp 220Centaurus AFornax AHE0450-2958IC 1459Messier 31 (or the Andromeda Galaxy) • Messier 32Messier 51 (or the Whirlpool Galaxy) • Messier 60Messier 77Messier 81 (or Bode's Galaxy) • Messier 84Messier 104 (or the Sombrero Galaxy) • Messier 105Messier 106Quiescent (Galaxy) (Black Hole at the center of the Andromeda Galaxy) • Mrk 421Mrk 501NGC 821NGC 1023NGC 1097NGC 1271NGC 1277NGC 1332NGC 1566NGC 2787NGC 3079NGC 3115NGC 3377NGC 3384NGC 3998NGC 4151NGC 4261NGC 4438NGC 4459NGC 4473NGC 4486B (a satellite galaxy of Messier 87) • NGC 4564NGC 4579NGC 4596NGC 4697NGC 4889NGC 4945NGC 5033NGC 6251NGC 7052NGC 7314PKS 0521-365PōniuāʻenaPōwehi (or Messier 87, Virgo A) • Q0906+6930 (a blazar organized around a supermassive black hole) • RX J1131 (first black hole whose spin was directly measured) • Sagittarius A*, which is at the center of the Milky Way TypesQuasarSupermassive black holeHypercompact stellar system (hypothetical object organized around a supermassive black hole) ==Intermediate-mass black holes and candidates==
Intermediate-mass black holes and candidates
Cigar Galaxy (Messier 82, NGC 3034) • GCIRS 13EHLX-1M82 X-1Messier 15 (NGC 7078) • Messier 110 (NGC 205) • Sculptor Galaxy (NGC 253) • Triangulum Galaxy (Messier 33, NGC 598) ==Stellar black holes and candidates==
Stellar black holes and candidates
1E1740.7-2942 (Great Annihilator), 340 ly from Sgr A*4U 1543-475/IL LupiA0620-00/V616 Mon (once thought to be the closest to Earth known, at about 3,000 light years) • CXOU J132527.6-430023 (a candidate stellar mass black hole outside of the Local Group) • Cygnus X-1Cygnus X-3GRO J0422+32 (possibly the smallest black hole yet discovered) • GRO J1655-40/V1033 Sco (at one time considered the smallest black hole known) • M33 X-7 (stellar black hole with the most massive stellar companion, located in the Triangulum Galaxy) • MOA-2011-BLG-191/OGLE-2011-BLG-0462 (first known isolated stellar black hole) • SN 1997D (in NGC 1536) • SS 433V404 CygV PuppisXTE J1118+480/KV UMaXTE J1550-564/V381 NorXTE J1650-500 (at one time considered the smallest black hole known) • XTE J1819-254/V4641 SgrLMC X-1 (first X-ray source in the Large Magellanic Cloud) • Gaia BH1Gaia BH2Gaia BH3 Black holes detected by gravitational wave signals , 10 mergers of binary black holes have been observed. In each case two black holes merged to a larger black hole. In addition, one neutron star merger has been observed (GW170817), forming a black hole. In addition, over 30 alerts have been issued since April 2019, of black hole merger candidates. • GW 150914 ==Multiple black hole systems==
Multiple black hole systems
Binary black holesEGSD2 J142033.66 525917.5 core black holes — galaxy hosting a dual AGN • OJ 287 core black holes — a BL Lac object with a candidate binary supermassive black hole core system • PG 1302-102 – the first binary-cored quasar — a pair of supermassive black holes at the core of this quasar • SDSS J120136.02+300305.5 core black holes — a pair of supermassive black holes at the centre of this galaxy In addition, the signal of several binary black holes merging into a single black hole and in so doing producing gravitational waves have been observed by the LIGO instrument. These are listed above in the section Black holes detected by gravitational wave signals. Trinary black holes As of 2014, there are 5 triple black hole systems known. • SDSS J150243.09+111557.3 (SDSS J1502+1115) core black holes — the three components are distant tertiary J1502P, and the close binary pair J1502S composed of J1502SE and J1502SW • 2MASX J10270057+1749001 (SDSS J1027+1749) core black holes ==See also==
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