Neutron stars are the gravitational collapsed core of massive stars (9-10 solar masses) that have gone supernova. [1] They are some of the densest objects in the universe only being surpassed by black holes. They generally have masses in the order of 1.5 solar masses compact into an area of just 12 kilometers. [2] Currently the largest neutron stars that has been discovered is PSR J1748-2021B which has a mass of 2.5 solar masses.
Below is a list of high-mass neutron stars.
| Name | Mass (M☉) | Distance (ly) | Companion class | Mass determination method | Notes | Refs. |
|---|---|---|---|---|---|---|
| PSR J1748-2021B | 2.548+0.047 −0.078 | 27,700 | D | Rate of advance of periastron. | In globular cluster NGC 6440. | [3] [1] [2] [4] |
| 4U 1700-37 | 2.44±0.27 | 6,910 ± 1,120 | O6.5Iaf+ | Monte Carlo simulations of thermal comptonization process. | HMXB system. | [5] [6] |
| PSR J2017-1614 | 2.4±0.6 | 4,570 | Substellar object | Black widow pulsar, in a tight 2.3 hour binary. | [7] | |
| PSR J0952–0607 | 2.35±0.17 | 3,200–5,700 | Substellar object | Radio-measured Shapiro delay | Black widow pulsar. Fastest spinning galactic pulsar. | [8] |
| PSR J1311–3430 | 2.15–2.7 | 6,500–12,700 | Substellar object | Spectroscopic and photometric observation. | Black widow pulsar. | [9] [10] |
| PSR J1600−3053 | 2.3+0.7 −0.6 | 6,500 ± 1,000 | D | Fourier analysis of Shapiro delay's orthometric ratio. | [11] [12] | |
| PSR J2215+5135 | 2.27+0.17 −0.15 | 10,000 | G5V | Innovative measurement of companion's radial velocity. | Redback pulsar. | [13] |
| XMMU J013236.7+303228 | 2.2+0.8 −0.6 | 2,730,000 | B1.5IV | Detailed spectroscopic modelling. | In M33, HMXB system. | [14] |
| PSR J0751+1807 | 2.10±0.2 | 6,500 ± 1,300 | D | Precision pulse timing measurements of relativistic orbital decay. | [15] | |
| PSR J0740+6620 | 2.08±0.07 | 4,600 | D | Range and shape parameter of Shapiro delay. | Most massive neutron star with a well-constrained mass. | [16] [17] [18] |
| PSR J0348+0432 | 2.01±0.04 | 2,100 | D | Spectroscopic observation and orbital decay due to radiation of gravitational waves. | [11] [19] | |
| PSR J1518+0204B (M5B) | 1.981 | 24,500 | M6-8V? | In the globular cluster, M5. In a 7 day binary with a low-mass 0.11-0.13 M☉ red dwarf. | [20] | |
| PSR B1516+02B | 1.94+0.17 −0.19 | 24,500 | D | Rate of advance of periastron. | In globular cluster M5. | [11] [21] |
| PSR J1614−2230 | 1.908±0.016 | 3,900 | D | Range and shape parameter of Shapiro delay. | In Milky Way's galactic disk. | [11] [12] [22] |
| Vela X-1 | 1.88±0.13 | 6,200 ± 650 | B0.5Ib | Rate of advance of periastron. | Prototypical detached HMXB system. | [23] |
| PSR J2222–0137 | 1.831 | 871 | D | Companion is a white dwarf which is one of the most massive at 1.319 M☉ | [24] | |
| PSR B1957+20 | 1.81±0.17 | 6,500 | Substellar object | Rate of advance of periastron. | Prototype star of black widow pulsars. | [25] [26] [27] |
| SWIFT J1756.9-2508 | 1.8±0.4 | 26,100 | Substellar object | Hosts one planet, it is notable for orbiting its star in 54 minutes. | [28] [29] | |