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^[update], it is the farthest jet discovered with a redshift of 6.82.^[3]^[4]^[5]

References

^ "Astronomers Discover Most Distant Known Cosmic Jet". Sci News. Retrieved 9 March 2021.
^ 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. 804 (2). The American Astronomical Society: 118. arXiv:1503.04214. Bibcode:2015ApJ...804..118B. doi:10.1088/0004-637X/804/2/118. S2CID 54184153. Retrieved 9 March 2021.
^ 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. 909 (1). Harvard University: 80. arXiv:2103.03295. Bibcode:2021ApJ...909...80B. doi:10.3847/1538-4357/abe239. S2CID 232135300.
^ "The most distant radio-loud quasar discovered". Phsy. Phys.org. Retrieved 26 March 2021.
^ "Farthest Radio Loud Quasar Discovered". Florida News Times. 15 March 2021. Retrieved 26 March 2021.

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[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. 804 (2). The American Astronomical Society: 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. 909 (1). Harvard University: 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.

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See also

References