Daftar lubang hitam paling masif

Berikut ini adalah sebuah daftar dari lubang hitam paling masif yang sejauh ini ditemukan (dan kandidat-kandidatnya), yang diukur dalam satuan massa matahari (), sekitar .

 Daftar 

+ Daftar lubang hitam tersupermasif Nama Massa matahari(Matahari = 1) Catatan TON 618   Perkiraan dari korelasi garis emisi kuasar Hβ.Holmberg 15A   Mass specified obtained through orbit-based, axisymmetric Schwarzschild models. Earlier estimates range from ~310 billion  down to 3 billion , all relying on empirical scaling relations and are thus obtained from extrapolation and not from kinematical measurements. IC 1101    Perkiraan dari properti galaksi induk; massa belum diukur secara langsung.S5 0014+81   Sebuah makalah 2010 mengusulkan bahwa sebuah corong mengkolimasi radiasi di sekitar sumbu jet, menciptakan ilusi optik dengan kecerahan sangat tinggi, dan dengan demikian kemungkinan terjadi sebuah overestimasi pada massa lubang hitam tersebut.SMSS J215728.21-360215.1   SDSS J102325.31+514251.0   Perkiraan dari korelasi garis emisi quasar MgII.H1821+643    Gugus galaksi terdekat yang mempunyai sebuah kuasar dalam intinya.NGC 6166   APM 08279+5255    Based on velocity width of CO line from orbiting molecular gas, and reverberation mapping using SiIV and CIV emission lines.NGC 4889  Best fit: the estimate ranges from 6 billion to 37 billion .Central black hole of Phoenix Cluster   This black hole is continuously growing at the rate of ~60  per year. SDSS J074521.78+734336.1   Estimated from quasar MgII emission line correlation.OJ 287 primary    A smaller 100 million  black hole orbits this one in a 12-year period (see OJ 287 secondary below). But this measurement is in question due to the limited number and precision of observed companion orbits. NGC 1600   Unprecedentedly massive in relation of its location: an elliptical galaxy host in a sparse environment. SDSS J08019.69+373047.3   Estimated from quasar MgII emission line correlation. SDSS J115954.33+201921.1   Estimated from quasar MgII emission line correlation. SDSS J075303.34+423130.8   Estimated from quasar Hβ emission line correlation. SDSS J080430.56+542041.1   Estimated from quasar MgII emission line correlation. Abell 1201 BCG  Estimated from the strong gravitational lensing of a background galaxy behind the BCG. Beware of ambiguity between the BH mass determination and the galaxy cluster's dark matter profile. SDSS J0100+2802   Estimated from quasar MgII emission line correlation. This object grew early in cosmic history (redshift 6.30). SDSS J081855.77+095848.0   Estimated from quasar MgII emission line correlation. NGC 1270   Elliptical galaxy located in the Perseus Cluster. Also is a low-luminosity AGN (LLAGN). SDSS J082535.19+512706.3   Estimated from quasar Hβ emission line SDSS J013127.34-032100.1    Estimated from accretion disk spectrum modelling. PSO J334.2028+01.4075    There are actually two black holes, orbiting at each other in a close pair with a 542-day period. The largest one is quoted, while the smaller one's mass is not defined.Black hole of central elliptical galaxy of RX J1532.9+3021    QSO B2126-158    NGC 1281    Compact elliptical galaxy in the Perseus Cluster. Mass estimates range from 10 billion  down to <5 billion . SDSS J015741.57-010629.6   NGC 3842   Brightest galaxy in the Leo Cluster SDSS J230301.45-093930.7   Estimated from quasar MgII emission line correlation. SDSS J075819.70+202300.9   Estimated from quasar Hβ emission line correlation. CID-947   Constitutes 10% of the total mass of its host galaxy. Estimated from quasar Hβ emission line correlation. SDSS J080956.02+502000.9   Estimated from quasar Hβ emission line correlation. SDSS J014214.75+002324.2   Estimated from quasar MgII emission line correlation. Messier 87 "Powehi" 
  Central galaxy of the Virgo Cluster; the first black hole directly imaged. NGC 5419   Estimated from the stellar velocity distribution. A secondary satellite SMBH may orbit around 70 parsecs. SDSS J025905.63+001121.9   Estimated from quasar Hβ emission line correlation. SDSS J094202.04+042244.5   Estimated from quasar Hβ emission line correlation. QSO B0746+254   QSO B2149-306   SDSS J090033.50+421547.0   Estimated from quasar MgII emission line correlation.Messier 60   SDSS J011521.20+152453.3   Estimated from quasar Hβ emission line correlation. QSO B0222+185  Hercules A (3C 348)    Notable for its million light-year long relativistic jet. Abell 1836-BCG    SDSS J213023.61+122252.0   Estimated from quasar Hβ emission line correlation. SDSS J173352.23+540030.4  Estimated from quasar MgII emission line correlation. SDSS J025021.76-075749.9  Estimated from quasar MgII emission line correlation. NGC 1271   Compact elliptical or lenticular galaxy in the Perseus Cluster. SDSS J030341.04-002321.9   Estimated from quasar MgII emission line correlation. QSO B0836+710    SDSS J224956.08+000218.0   Estimated from quasar Hβ emission line correlation. SDSS J030449.85-000813.4   Estimated from quasar Hβ emission line correlation. SDSS J234625.66-001600.4   Estimated from quasar Hβ emission line correlation. PKS 2128-123    ULAS J1120+0641     QSO 0537-286   NGC 3115    Q0906+6930    Most distant blazar, at z = 5.47 QSO B0805+614   Messier 84    J100758.264+211529.207 ("Pōniuāʻena")    Second most-distant quasar known PKS 2059+034   Abell 3565-BCG  NGC 7768  NGC 1277   Once thought to harbor a black hole so large that it contradicted modern galaxy formation and evolutionary theories, re-analysis of the data revised it downward to roughly a third of the original estimate. and then one tenth.Black hole of central elliptical galaxy of MS 0735.6+7421    Produced a colossal AGN outburst after accreting 600 million  worth of material. BH mass not explicitly stated; just a lower limit. Requires assumptions about the efficiencies of gas accretion and jet power.Most Powerful Eruption In The Universe Discovered NASA/Marshall Space Flight Center (ScienceDaily) January 6, 2005 QSO B225155+2217    QSO B1210+330    NGC 6166    Central galaxy of Abell 2199; notable for its hundred thousand light year long relativistic jet. Cygnus A    Brightest extrasolar radio source in the sky as seen at frequencies above 1 GHz Sombrero Galaxy    Bolometrically most luminous galaxy in the local universe and also the nearest billion-solar-mass black hole to Earth. Markarian 501  –  Brightest object in the sky in very high energy gamma rays. PG 1426+015    3C 273    Kuasar terterang di langit ULAS J1342+0928    Kuasar paling jauh − saat ini tercatat sebagai kuasar terjauh dengan z=7.54 Messier 49    NGC 1399    Central galaxy of the Fornax Cluster PG 0804+761    PG 1617+175    PG 1700+518    NGC 4261    Notable for its  light-year long relativistic jet. PG 1307+085  281 840 000  SAGE0536AGN   Constitutes 1.4% of the mass of its host galaxy NGC 1275    Central galaxy of the Perseus Cluster 3C 390.3    II Zwicky 136    PG 0052+251    Messier 59    Lubang hitam tersebut memiliki sebuah rotasi retrograd. PG 1411+442    Markarian 876    Galaksi Andromeda   Galaksi besar terdekat ke Bima Sakti PG 0953+414    PG 0026+129    Fairall 9    Markarian 1095    Messier 105  – Markarian 509    Sekunder dari OJ 287    The smaller black hole orbiting OJ 287 primary (see above). RX J124236.9-111935    Observed by the Chandra X-ray Observatory to be tidally disrupting a star.NASA: "Giant Black Hole Rips Apart Unlucky Star" Messier 85   NGC 5548    PG 1211+143    Messier 88    Messier 81 (Galaksi Bode)    Markarian 771    Messier 58    PG 0844+349    Centaurus A    Also notable for its million light-year long relativistic jet. Markarian 79    Messier 96    Estimates can be as low as 1.5 million solar masses Markarian 817   NGC 3227   NGC 4151 primary    3C 120    Markarian 279    NGC 3516    NGC 863    Messier 82 (Cigar Galaxy)    Prototype starburst galaxy. Messier 108    M60-UCD1    Constitutes 15% of the mass of its host galaxy. NGC 3783    Markarian 110    Markarian 335    NGC 4151 secondary    NGC 7469    IC 4329 A    NGC 4593    Messier 61    Messier 32  –
  Sebuah galaksi satelit katai di Galaksi Andromeda. Sagittarius A*    Lubang hitam di pusat Bima Sakti.

 Lihat pula 

 Daftar struktur kosmik terbesar
 Daftar galaksi terbesar
 Daftar lubang hitam paling tidak masif
 Daftar eksoplanet paling masif

 Referensi 

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Kategori:Daftar bertopik astronomi