6C B133058.8+575451

6C B133058.8+575451
SDSS image of 6C B133058.8+575451
Observation data (J2000.0 epoch)
ConstellationUrsa Major
Right ascension13h 32m 50.65s[1]
Declination+57° 39′ 41.90″[1]
Redshift0.301091[1]
Heliocentric radial velocity90265 ± 46 km/s[1]
Distance4,348.2 ± 304.4 Mly (1,333.15 ± 93.33 Mpc)[1]
Group or clusterAbell 1761 (WHL J133250.7+573942)
magnitude (J)14.61[1]
Characteristics
TypeAGN[1]
Size~713,000 ly (218.7 kpc) (estimated)[1]
Other designations
2MASX J13325065+5739418, SDSS J133250.67+573941.6, LEDA 2569523, [YCH2015] J203.2111+57.6616, [YHW2016] J203.21107+57.66164, WHL J133250.7+573942 BCG[1]

6C B133058.8+575451 is a radio galaxy located in the constellation of Ursa Major. The redshift of the galaxy is (z) 0.301[1] and it was first discovered by astronomers in July 1993.[2]

Description

6C B133058.8+575451 is the brightest cluster galaxy of the Abell 1761 galaxy cluster,[3] which is also known as WHL J133250.7+573942, with 50 confirmed galaxy member candidates. The R-band magnitude of the galaxy is 16.91 while its absolute magnitude is-24.19.[4][5] The infrared J-band and H-band magnitudes are estimated to be 16.12 and 15.47 respectively.[6]

The optical spectrum of the galaxy has presence of both hydrogen-alpha and doubly ionized oxygen emission lines with estimated line luminosities of 0.000 and 7.340 L☉. A supermassive black hole is located in the center of the galaxy with mass of 8.77 M☉.[7]

The nucleus is found to be active and it is classified as a Fanaroff-Riley Class Type II radio galaxy with its estimated flux density of 228.00 mJy by NRAO VLA Sky Survey (NVSS) at 1.4 GHz frequencies.[8] The radio lobes are resolved and they have a total lobe size of 33.55 kiloparsecs in total. The angular size of the source is 15.14 arcseconds while the total log 1.4 GHz radio luminosity is 26.29 WHz−1.[7] There is also a presence of a radio jet whose jet power is calculated to be 45.23 erg s−1 whereas the accretion disk luminosity is 0.000 erg s−1.[9] Radio imaging made with Very Large Array (VLA) at 20 centimeters found the radio flux density at 1400 MHz is 221 mJy while its absolute radio luminosity at 1400 MHz is 25.43 W Hz−1.[10]

References

  1. 1 2 3 4 5 6 7 8 9 10 "NED Search results for 6C B133058.8+575451". NASA/IPAC Extragalactic Database. Retrieved 2026-07-13.
  2. ↑ Owen, Frazer N.; White, Richard A.; Ge, Jingping (July 1993). "A 20 centimeter VLA survey of Abell clusters of galaxies. III - Images and optical identifications". The Astrophysical Journal Supplement Series. 87: 135. Bibcode:1993ApJS...87..135O. doi:10.1086/191800. ISSN 0067-0049.
  3. ↑ Ledlow, Michael J.; Owen, Frazer N. (November 1995). "A 20 CM Survey of Abell Clusters of Galaxies. V. Optical Observations and Surface Photometry". The Astronomical Journal. 110: 1959. Bibcode:1995AJ....110.1959L. doi:10.1086/117663. ISSN 0004-6256.
  4. ↑ Wen, Z. L.; Han, J. L.; Liu, F. S. (2012-03-30). "A Catalog of 132,684 Clusters of Galaxies Identified from Sloan Digital Sky Survey III". The Astrophysical Journal Supplement Series. 199 (2): 34. arXiv:1202.6424. Bibcode:2012ApJS..199...34W. doi:10.1088/0067-0049/199/2/34. ISSN 0067-0049.
  5. ↑ Yuan, Z. S.; Han, J. L.; Wen, Z. L. (2016-05-12). "Radio luminosity function of brightest cluster galaxies". Monthly Notices of the Royal Astronomical Society. 460 (4): 3669–3678. arXiv:1605.03387. doi:10.1093/mnras/stw1125. ISSN 0035-8711.
  6. ↑ Yang, Xiao-hong; Chen, Pei-sheng; Huang, Yan (2015-04-08). "Infrared colour properties of nearby radio-luminous galaxies". Monthly Notices of the Royal Astronomical Society. 449 (3): 3191–3201. arXiv:1502.05800. doi:10.1093/mnras/stv460. ISSN 1365-2966.
  7. 1 2 Sikora, Marek; Stasińska, Grażyna; Kozieł-Wierzbowska, Dorota; Madejski, Greg M.; Asari, Natalia V. (2013-02-15). "Constraining Jet Production Scenarios by Studies of Narrow-Line Radio Galaxies". The Astrophysical Journal. 765 (1): 62. arXiv:1210.2571. Bibcode:2013ApJ...765...62S. doi:10.1088/0004-637x/765/1/62. ISSN 0004-637X.
  8. ↑ Ma, Zhixian; Xu, Haiguang; Zhu, Jie; Hu, Dan; Li, Weitian; Shan, Chenxi; Zhu, Zhenghao; Gu, Liyi; Li, Jinjin; Liu, Chengze; Wu, Xiangping (2019-02-01). "A Machine Learning Based Morphological Classification of 14,245 Radio AGNs Selected from the Best–Heckman Sample". The Astrophysical Journal Supplement Series. 240 (2): 34. arXiv:1812.07190. Bibcode:2019ApJS..240...34M. doi:10.3847/1538-4365/aaf9a2. ISSN 0067-0049.
  9. ↑ Rusinek, Katarzyna; Sikora, Marek; Kozieł-Wierzbowska, Dorota; Godfrey, Leith (2016-12-23). "On the efficiency of jet production in FR II radio galaxies and quasars". Monthly Notices of the Royal Astronomical Society. 466 (2): 2294–2301. arXiv:1612.07392. doi:10.1093/mnras/stw3330. ISSN 0035-8711.
  10. ↑ Owen, Frazer N.; Ledlow, Michael J. (1997). "A 20 Centimeter VLA Survey of Abell Clusters of Galaxies. VII. Detailed Radio Images". The Astrophysical Journal Supplement Series. 108 (1): 41–98. Bibcode:1997ApJS..108...41O. doi:10.1086/312954. ISSN 0067-0049.
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