PSO J172.3556+18.7734

PSO J172.3556+18.7734 is an astrophysical jet that was discovered in May 2011. It was originally thought to be a quasar by astronomers, but as of March 8, 2021, it is now classified as a cosmic jet (astrophysical jet).[1][2] As of 2021, it is the farthest radio-loud quasar discovered with a redshift of 6.82.[3][4][5]

See also

References
  1. "Astronomers Discover Most Distant Known Cosmic Jet". Sci News. Retrieved 9 March 2021.
  2. Bañados, E.; Venemans, B. P.; Morganson, E.; Hodge, J.; Decarli, R.; Walter, F.; Stern, D.; Schlafly, E.; Farina, E. P.; Greiner, J.; Chambers, K. C.; Fan, X.; Rix, H-W.; Burgett, W. S.; Draper, P. W.; Flewelling, J.; Kaiser, N.; Metcalfe, N.; Morgan, J. S.; Tonry, J. L.; Wainscoat, R. J. (2015). "CONSTRAINING THE RADIO-LOUD FRACTION OF QUASARS AT z > 5.5". The Astrophysical Journal. The American Astronomical Society. 804 (2): 118. arXiv:1503.04214. Bibcode:2015ApJ...804..118B. doi:10.1088/0004-637X/804/2/118. S2CID 54184153. Retrieved 9 March 2021.
  3. Bañados, Eduardo; Mazzucchelli, Chiara; Momjian, Emmanuel; Eilers, Anna-Christina; Wang, Feige; Schindler, Jan-Torge; Connor, Thomas; Andika, Irham Taufik; Barth, Aaron J.; Carilli, Chris; Davies, Frederick B.; Decarli, Roberto; Fan, Xiaohui; Farina, Emanuele Paolo; Hennawi, Joseph F.; Pensabene, Antonio; Stern, Daniel; Venemans, Bram P.; Wenzl, Lukas; Yang, Jinyi (2021). "The Discovery of a Highly Accreting, Radio-loud Quasar at z = 6.82". The Astrophysical Journal. Harvard University. 909 (1): 80. arXiv:2103.03295. Bibcode:2021ApJ...909...80B. doi:10.3847/1538-4357/abe239. S2CID 232135300.
  4. "The most distant radio-loud quasar discovered". Phsy. Phys.org. Retrieved 26 March 2021.
  5. "Farthest Radio Loud Quasar Discovered". Florida News Times. 15 March 2021. Retrieved 26 March 2021.


This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.