數(shù)據(jù)大部分來自維基條目:list of most masive? ?black holes? ? 部分來自于相關(guān)論文

質(zhì)量≤100億M⊙的黑洞選擇部分收錄，天體簡(jiǎn)介內(nèi)容使用原文

太陽質(zhì)量=?1M⊙(1.89*103okg)

銀河系質(zhì)量≈5*1011M⊙

地球質(zhì)量≈0.000003M⊙

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Phoenix A

質(zhì)量:1*1011M⊙

簡(jiǎn)介:Estimated using a calorimetric model on the adiabatic behavior of core regrowth and an assumed core-Sérsic model of n=4. It is consistent with evolutionary modelling of gas accretion and the dynamics and density profiles of the galaxy.?Mass has not been measured directly

4C +74.13

質(zhì)量:5.13(+9.66/-3.35)*101oM⊙

簡(jiǎn)介:Produced a colossal AGN outburst after accreting 600 million?M☉?worth of material.

Estimated using the break radius of 0.5 kpc core of the central galaxy.?Previous indirect assumptions about the efficiencies of gas accretion and jet power yield a lower limit of 1 billion?M☉.

現(xiàn)宇宙演化階段黑洞理論質(zhì)量上限:5×101oM⊙

TON 618

質(zhì)量:4.07*101oM⊙

簡(jiǎn)介:Estimated from quasar Hβ emission line correlation.

Holmberg 15A

質(zhì)量:(4.0±0.8)*101oM⊙

簡(jiǎn)介:Mass specified obtained through orbit-based, axisymmetric Schwarzschild models. Earlier estimates range from ~310 billion?M☉?down to 3 billion?M☉, all relying on empirical scaling relations and are thus obtained from extrapolation and not from kinematical measurement.

IC 1101

質(zhì)量:(4-10)*101oM⊙

簡(jiǎn)介:Estimated from properties of the host galaxy; mass has not been measured directly.

S5 0014+81

質(zhì)量:4*101oM⊙

簡(jiǎn)介:A 2010 paper suggested that a funnel collimates the radiation around the jet axis, creating an optical illusion of very high brightness, and thus a possible overestimation of the black hole mass.

SMSS J215728.21-360215.1

質(zhì)量:(3.4±0.6)*101oM⊙

SDSS J102325.31+514251.0

質(zhì)量:(3.31±0.61)*101oM⊙

簡(jiǎn)介:Estimated from quasar MgII emission line correlation.

H1821+643

質(zhì)量:3*101oM⊙

簡(jiǎn)介:Value obtained as an indirect estimate using a model of minimum Eddington luminosity required to account for the Compton cooling of the surrounding cluster.

NGC 6166

質(zhì)量:3×101oM⊙

簡(jiǎn)介:Central galaxy of?Abell 2199; notable for its hundred thousand light year long relativistic jet.

APM 08279+5255

質(zhì)量:2.3×101oM⊙或(1.02±0.15)×101oM⊙

簡(jiǎn)介:Based on velocity width of CO line from orbiting molecular gas,?and?reverberation mapping?using SiIV and CIV emission lines.

NGC 4889

質(zhì)量:(2.1±1.6)×101oM⊙

簡(jiǎn)介:Best fit: the estimate ranges from 6 billion to 37 billion?M☉.

Central black hole of?Phoenix Cluster

質(zhì)量:2×101oM⊙

簡(jiǎn)介:This black hole is continuously growing at the rate of ~60?M☉?per year.

SDSS J074521.78+734336.1

質(zhì)量:(1.95±0.05)×101oM⊙

簡(jiǎn)介:Estimated from quasar MgII emission line correlation.

OJ 287

質(zhì)量:1.8×101oM⊙

簡(jiǎn)介:OJ 287(SMBH) is aextremely?large black hole,A?smaller 100 million?M☉?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

質(zhì)量:(1.7±0.15)×101oM⊙

簡(jiǎn)介:Unprecedentedly massive in relation of its location: an elliptical galaxy host in a sparse environment.

SDSS J08019.69+373047.3

質(zhì)量:(1.51±0.31)×101oM⊙

簡(jiǎn)介:Estimated from quasar MgII emission line correlation.

SDSS J115954.33+201921.1

質(zhì)量:(1.41±0.10)×101oM⊙

簡(jiǎn)介:Estimated from quasar MgII emission line correlation.

SDSS J075303.34+423130.8

質(zhì)量:(1.38±0.03)×101oM⊙

簡(jiǎn)介:Estimated from quasar Hβ emission line correlation.

SDSS? J080430.56+542041.1

質(zhì)量:(1.35±0.22)×101oM⊙

簡(jiǎn)介:Estimated from quasar MgII emission line correlation.

Abell 1201 BCG

質(zhì)量:(1.3±0.6)×101oM⊙

簡(jiǎn)介: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

質(zhì)量:(1.24±0.19)×101oM⊙

簡(jiǎn)介:Estimated from quasar MgII emission line correlation. This object grew early in cosmic history (redshift?6.30).

SDSS J081855.77+095848.0

質(zhì)量:(1.20±0.06)×101oM⊙

簡(jiǎn)介:Estimated from quasar MgII emission line correlation.

NGC 1270?

質(zhì)量:1.2×101oM⊙

簡(jiǎn)介:Elliptical galaxy located in the?Perseus Cluster. Also is a low-luminosity?AGN?(LLAGN).

SDSS J082535.19+512706.3

質(zhì)量:(1.12±0.20)×101oM⊙

簡(jiǎn)介:Estimated from quasar Hβ emission line.

SDSS J013127.34-032100.1

質(zhì)量:(1.1±0.2)×101oM⊙

簡(jiǎn)介:Estimated from accretion disk spectrum modelling.

PSO J334.2028+01.4075

?質(zhì)量:101oM⊙

簡(jiǎn)介: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.

RX J1532.9+3021

質(zhì)量:101oM⊙

QSO B2126-158

質(zhì)量:101oM⊙

NGC 1281

質(zhì)量:101oM⊙

簡(jiǎn)介:Compact?elliptical galaxy?in the?Perseus Cluster. Mass estimates range from 10 billion?M☉?down to <5 billion?M☉

質(zhì)量≤100億M⊙的部分黑洞

?.SDSS J140821.67+025733.2

質(zhì)量:8 000 000 000M⊙

?.M87

質(zhì)量:(7.2±3.6)×1 000 000 000M⊙

?.Hercules A?(3C 348)

質(zhì)量:4 000 000 000M⊙

?.NGC 6166

質(zhì)量:1 000 000 000M⊙

?.人馬座A*

質(zhì)量:4?000 000M⊙

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維基列表未收錄的特大質(zhì)量黑洞

QSO J084538.66+342043.6

質(zhì)量:1.64*101oM⊙

來源:https://doi.org/10.1111/j.1365-2966.2010.18099.x

PG 0050+124

質(zhì)量:≧101oM⊙

來源:

NEAR-INFRARED ADAPTIVE OPTICS IMAGING OF QSO HOST GALAXIES

IRAS F

質(zhì)量:101oM⊙

來源:

CATALOG OF SUPERMASSIVE BLACK HOLES FOR INTERFEROMETRIC OBSERVATIONS

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更新記錄:

創(chuàng)建日期:2021.4.2

更新日期:2021.4.8(NGC6166簡(jiǎn)介變動(dòng))

更新日期:2021.4.11(SDSS J073739.96+384413.2，SDSS?J132624.76+131727.4，SDSS?J221511.93-004550.0，SDSS?J014036.47+000335.8信息刪除?)

更新日期:2021.4.14(OJ 287信息補(bǔ)充)

更新日期:2021.4.15(RBS 2043信息補(bǔ)充)

更新日期:2021.4.18(H1821+643信息修改)

更新日期:2021.6.8(添加IRIS-F)

更新日期:2022.10.18(刪除Central black hole of?Phoenix Cluster.RBS 2043.增加Phoenix,

4C +74.13)

更新日期:2023.1.22(TON618數(shù)據(jù)下調(diào))