Quasar in the constellation of Coma Berenices
3C 275.1 is aquasar located in theconstellation ofComa Berenices with aredshift of (z) 0.555.[ 1] astronomers , and is situated in the center of a richgalaxy cluster .[ 2] elliptical galaxy , described as either a proto-cD orType-cD galaxy with an emissionnebula surrounding it.[ 3] [ 4] [ 5]
3C 275.1 is classified as agamma-ray lobe-dominated quasar.[ 6] jet heading in northwards direction based on a super-resolved radio imaging made by theVery Long Baseline Array (VLBA).[ 7] GHz with a 5-kilometertelescope shows 3C 275.1 to contain a double component showing one side as compact and the other being slightly extended.[ 8] interacting with a companion galaxy.[ 9] [ 10]
Observations made in 1986 revealed the presence of a rotatinggas cloud around 3C 275.1 with adiameter of more than 100kiloparsecs (Kpc). Based on observations, it was found to be the largest known to surround a quasar and is likely remnants created bytidal interactions or material that is accumulated viacooling flows originating from the cluster.[ 11] ionized gas tails that extends up to 170 kiloparsecs, typical ofJellyfish galaxies .[ 12] conical shape with a bar-shaped extension that is located southwards from the nucleus[ 13] X-ray emission of 7.6 x 1043 erg s−1 .[ 14]
In the center of 3C 275.1, there is asupermassive black hole estimated to have a mass of about 200 millionsolar masses based on a black hole-spheroid mass ratio calculated foractive galactic nuclei .[ 15] [ 12] NGC 4651 , due to the radio emitter alignment at the rear of the latter's outergalactic disk .[ 16]
^ Liu, Ronghui; Pooley, Guy (1990-07-01)."Radio polarization and the environment of 3C 275.1" .Monthly Notices of the Royal Astronomical Society .245 : 17P.Bibcode :1990MNRAS.245P..17L .ISSN 0035-8711 . ^ Krempec-Krygier, J.; Krygier, B.; Walentynowicz, G. (1998-06-01)."The group of galaxies around 3C 275.1" .Astronomy and Astrophysics .334 :427– 438.Bibcode :1998A&A...334..427K .ISSN 0004-6361 . ^ Hintzen, Paul; Romanishin, W. (1986-12-01)."Direct Imaging of the Extremely Large Host Galaxy and Gas Cloud Surrounding the Quasar 3C 275.1" .The Astrophysical Journal .311 : L1.Bibcode :1986ApJ...311L...1H .doi :10.1086/184787 .ISSN 0004-637X . ^ Hintzen, P.; Boeshaar, G. O.; Scott, J. S. (1981-05-01)."Detection of an apparent, distant cluster of galaxies associated with the radio-tail QSO 3C 275.1" .The Astrophysical Journal .246 :L1 – L4 .Bibcode :1981ApJ...246L...1H .doi :10.1086/183541 .ISSN 0004-637X . ^ Crawford, C. S.; Lehmann, I.; Fabian, A. C.; Bremer, M. N.; Hasinger, G. (1999-10-01)."Detection of X-ray emission from the host clusters of 3CR quasars" .Monthly Notices of the Royal Astronomical Society .308 (4):1159– 1172.arXiv :astro-ph/9904371 Bibcode :1999MNRAS.308.1159C .doi :10.1046/j.1365-8711.1999.02804.x ISSN 0035-8711 . ^ Liao, Neng-Hui; Xin, Yu-Liang; Li, Shang; Jiang, Wei; Liang, Yun-Feng; Li, Xiang; Zhang, Peng-Fei; Chen, Liang; Bai, Jin-Ming; Fan, Yi-Zhong (2015-07-17)."DISCOVERY OFγ -RAY EMISSION FROM THE STRONGLY LOBE-DOMINATED QUASAR 3C 275.1" .The Astrophysical Journal .808 (1): 74.arXiv :1501.00635 doi :10.1088/0004-637x/808/1/74 .ISSN 1538-4357 . ^ Hough, D. H.; Vermeulen, R. C.; Readhead, A. C. S.; Cross, L. L.; Barth, E. L.; Yu, L. H.; Beyer, P. J.; Phifer, E. M. (2002-03-01)."Parsec-Scale Radio Structure and Broad Optical Emission Lines in a Complete Sample of 3CR Lobe-dominated Quasars" .The Astronomical Journal .123 (3):1258– 1287.Bibcode :2002AJ....123.1258H .doi :10.1086/338847 .ISSN 0004-6256 . ^ Riley, J. M.; Pooley, G. G. (1978-09-01)."15-GHz observations of the quasars 3C 270.1 and 3C 275.1" .Monthly Notices of the Royal Astronomical Society .184 (4):769– 772.doi :10.1093/mnras/184.4.769 ISSN 0035-8711 . ^ Liu, R.; Pooley, G.; Riley, J. M. (1992-08-15)."Spectral ageing in a sample of 14 high-luminosity double radio sources" .Monthly Notices of the Royal Astronomical Society .257 (4):545– 571.Bibcode :1992MNRAS.257..545L .doi :10.1093/mnras/257.4.545 ISSN 0035-8711 . ^ Rector, Travis A.; Stocke, John T.; Ellingson, Erica (1995-10-01)."Quasar Radio Morphology and Clustering Environment at z~1/2" .The Astronomical Journal .110 : 1492.Bibcode :1995AJ....110.1492R .doi :10.1086/117622 .ISSN 0004-6256 . ^ Hintzen, P.; Stocke, J. (1986-09-01)."Detection of aRotating Gas Cloud 100 Kiloparsecs in Diameter Surrounding 3C 275.1, a Quasar at the Center of a Rich Cluster of Galaxies" .The Astrophysical Journal .308 : 540.Bibcode :1986ApJ...308..540H .doi :10.1086/164524 .ISSN 0004-637X . ^a b Zhao, Qinyuan; Wang, Junfeng; Li, Zhenzhen (2024-08-01)."Serendipitous Catch of a Giant Jellyfish: An Ionized Nebula around 3C 275.1 with 170 kpc Long Tails" .The Astrophysical Journal .971 (2): 134.arXiv :2406.11433 Bibcode :2024ApJ...971..134Z .doi :10.3847/1538-4357/ad58d6 ISSN 0004-637X . ^ McCarthy, Patrick J.; Spinrad, Hyron; van Breugel, Wil (July 1995)."Emission-Line Imaging of 3CR Radio Galaxies. I. Imaging Data" .The Astrophysical Journal Supplement Series .99 : 27.Bibcode :1996A&A...313..423H .doi :10.1086/192178 .ISSN 0067-0049 . ^ Crawford, C. S.; Fabian, A. C. (March 2003)."Extended X-ray emission around four 3C quasars at 0.55 > z < 0.75 observed with Chandra" .Monthly Notices of the Royal Astronomical Society .339 (4):1163– 1169.arXiv :astro-ph/0211232 Bibcode :2003MNRAS.339.1163C .doi :10.1046/j.1365-8711.2003.06268.x ISSN 0035-8711 . ^ McLure, R. J.; Jarvis, M. J.; Targett, T. A.; Dunlop, J. S.; Best, P. N. (2006-05-01)."On the evolution of the black hole: spheroid mass ratio" .Monthly Notices of the Royal Astronomical Society .368 (3):1395– 1403.arXiv :astro-ph/0510121 Bibcode :2006MNRAS.368.1395M .doi :10.1111/j.1365-2966.2006.10228.x ISSN 0035-8711 . ^ Schneider, Stephen E.; Corbelli, Edvige (1993-09-01)."Neutral Hydrogen Absorption and Emission in the Quasar/Galaxy Pair 3C 275.1/NGC 4651" .The Astrophysical Journal .414 : 500.arXiv :astro-ph/9307008 Bibcode :1993ApJ...414..500S .doi :10.1086/173097 .ISSN 0004-637X .
