Star in the constellation Microscopium
PSR J2124−3358 is a millisecond pulsar located in the constellation Microscopium . It is one of the brightest examples of its type in the X-ray spectrum. Discovered in 1997, no optical component was observed in 2003.[ 5]
References
^ a b Kerr, M.; Ray, P. S.; Johnston, S.; Shannon, R. M.; Camilo, F. (November 25, 2015). "Timing Gamma-ray Pulsars with the Fermi Large Area Telescope: Timing Noise and Astrometry" . The Astrophysical Journal . 814 (2). American Astronomical Society: 128. arXiv :1510.05099 . Bibcode :2015ApJ...814..128K . doi :10.1088/0004-637x/814/2/128 . ISSN 1538-4357 . S2CID 102342118 .
^ Abdo, A. A.; et al. (May 25, 2010). "Fermi Large Area Telescope First Source Catalog" . The Astrophysical Journal Supplement Series . 188 (2). American Astronomical Society: 405–436. arXiv :1002.2280 . Bibcode :2010ApJS..188..405A . doi :10.1088/0067-0049/188/2/405 . ISSN 0067-0049 . S2CID 122825311 .
^ Perera, B B P; et al. (October 12, 2019). "The International Pulsar Timing Array: second data release" . Monthly Notices of the Royal Astronomical Society . 490 (4). Oxford University Press (OUP): 4666–4687. arXiv :1909.04534 . Bibcode :2019MNRAS.490.4666P . doi :10.1093/mnras/stz2857 . ISSN 0035-8711 . S2CID 259278135 .
^ Hobbs, G.; Lorimer, D. R.; Lyne, A. G.; Kramer, M. (July 1, 2005). "A statistical study of 233 pulsar proper motions" . Monthly Notices of the Royal Astronomical Society . 360 (3). Oxford University Press (OUP): 974–992. arXiv :astro-ph/0504584 . Bibcode :2005MNRAS.360..974H . doi :10.1111/j.1365-2966.2005.09087.x . ISSN 0035-8711 . S2CID 18099069 .
^ a b Mignani, Roberto P.; Becker, Werner (2003). "VLT observations of the solitary millisecond pulsar PSR J2124 −3358". Advances in Space Research . 33 (4): 616–619. arXiv :astro-ph/0301114 . doi :10.1016/j.asr.2003.08.027 . S2CID 6841754 .