PSR J1748-2021B explained

PSR J1748-2021B
Event Type:Neutron star, binary pulsar
Class:Pulsar
Type:Binary pulsar
Start Time:March 2008
Discovery:Green Bank Telescope S-Band receiver
Duration:7514 and 4285 sec
Detected By:Green Bank Telescope
Constellation:Virgo
Ra:17h 48m 52.9522s (287.2205342 d)
Dec:−20h 21m 38.90s (−20.360881 d)
Epoch:2000
Gal:NGC 6440
Distance:223 pc
Source:SIMBAD
Snrtype:17
Host:https://simbad.u-strasbg.fr/simbad/sim-ref?bibcode=2008ApJ...675..670F
B-V:BRIGHT 2
Mag V:2.548 Solar mass
Names:NGC 6440B
Website:https://simbad.cds.unistra.fr/mobile/object.html?object_name=PSR%20J1748-2021B
Commons:NGC6440B

PSR J1748-2021B is the most massive known pulsar, initially calculated with . It was first discovered by Freire[1] using the Green Bank Telescope S band receiver and Pulsar Spigot Spectrometer in Terzan 5 of globular cluster M-5.[2]

A later estimate puts the mass as .[3]

Notes and References

  1. Freire . Paulo C. C. . Ransom . Scott M. . Bégin . Steve . Stairs . Ingrid H. . Hessels . Jason W. T. . Frey . Lucille H. . Camilo . Fernando . March 2008 . Eight New Millisecond Pulsars in NGC 6440 and NGC 6441 . The Astrophysical Journal . 675 . 1 . 670–682 . 10.1086/526338 . 0004-637X. 0711.0925 .
  2. Kumar . Sandeep S. . Kenath . Arun . Sivaram . C. . 2020-05-01 . Effects of dark matter on the upper bound mass of neutron stars . Physics of the Dark Universe . 28 . 100507 . 10.1016/j.dark.2020.100507 . 214343780 . 2212-6864.
  3. Long-Term Timing of Pulsars in NGC 6440: An Updated Mass Limit of Millisecond Pulsar J1748-2021B. Clifford. Nick. May 2019.