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PKS 1353−341

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PKS 1353−341
PKS 1353-341 captured by DESI Legacy Surveys
Observation data (J2000.0 (ICRS) epoch)
ConstellationCentaurus
Right ascension13h 56m 05.38657s[1]
Declination−34° 21′ 10.8591″[1]
Redshift0.222928[2]
Heliocentric radial velocity59,531±23 km/s[2]
Distance3.7228 Gly (1.14141 Gpc)[3]
Group or clusterPSZ2 G317.79+26.63[4]
Apparent magnitude (V)18.5[5]
Apparent magnitude (B)17.47[6]
Absolute magnitude (V)−22.4[3]
Characteristics
Typecompact dwarf galaxy[7] + Quasar[8]
Mass(30±1)×1010[3] M☉
Apparent size (V)0.267 × 0.144"[9]
Other designations
PGC 88936[10]

PKS 1353−341, also known as LEDA 88936 is a quasar (99% chance)[8] located in the southern constellation Centaurus. It has an apparent magnitude of 18.5, making it only visible in powerful telescopes. Based on the object's luminosity, it is estimated to be 3.7 billion light years distant from the Solar System. It is receding from the Milky Way with a heliocentric radial velocity of 59,531 km/s

The object was first identified by R.A. Preston in 1985.[11] Before then, it was unnoticed. Analysis in 1998 reveal that it might be relatively dusty based on the quasar's X-ray properties;[12] Long thought to be solitary, the CHiPS (Clusters Hiding in Plain Sight) Survey found PSZ2 G317.79+26.63, a massive galaxy cluster surrounding the quasar.[4] The team analyzed data from the 2MASS, NVSS, ROSAT, SUMSS, and WISE all-sky surveys in order to locate powerful sources of infrared, radio, and X-ray light. The goal was to discover new galaxy clusters that were previously misidentified as isolated sources of X-ray light due to the central quasar's brightness.[13][4]

As an individual object, PKS 1353−341 has a central mass 300 billion times that of the Sun,[3] which is 1/4 of the Milky Way's mass. It has an absolute magnitude of −22.4 in the blue passband,[3] making it very luminous. The galaxy hosting PKS 1353−341 is a compact dwarf galaxy.[7] Typical of quasars, PKS 1353−341 has two jets originating from the center of the galaxy. When combined with the surrounding cluster, both have a mass of 6.9+3.4
−2.6×1014 M☉, making it a thousand times more massive than our own galaxy.[4]

References

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  1. ^ a b Gordon, David; Jacobs, Christopher; Beasley, Anthony; Peck, Alison; Gaume, Ralph; Charlot, Patrick; Fey, Alan; Ma, Chopo; Titov, Oleg; Boboltz, David (27 May 2016). "SSecond Epoch VLBA Calibrator Survey Observations: VCS-II". The Astronomical Journal. 151 (6): 154. Bibcode:2016AJ....151..154G. doi:10.3847/0004-6256/151/6/154. eISSN 1538-3881. PMC 6010998. PMID 29937549.
  2. ^ a b Paturel, G.; Dubois, P.; Petit, C.; Woelfel, F. (2002). "Comparison LEDA/SIMBAD octobre 2002. Catalogue to be published in 2003". LEDA: 0. Bibcode:2002LEDA.........0P.
  3. ^ a b c d e Dálya, G; Díaz, R; Bouchet, F R; Frei, Z; Jasche, J; Lavaux, G; Macas, R; Mukherjee, S; Pálfi, M; de Souza, R S; Wandelt, B D; Bilicki, M; Raffai, P (30 May 2022). "GLADE+:an extended galaxy catalogue for multi-messenger searches with advanced gravitational-wave detectors". Monthly Notices of the Royal Astronomical Society. 514 (1): 1403–1411. arXiv:2110.06184. Bibcode:2022MNRAS.514.1403D. doi:10.1093/mnras/stac1443. eISSN 1365-2966. ISSN 0035-8711.
  4. ^ a b c d Somboonpanyakul, Taweewat; McDonald, Michael; Lin, Henry W.; Stalder, Brian; Stark, Antony (16 August 2018). "The Clusters Hiding in Plain Sight (CHiPS) Survey: A First Discovery of a Massive Nearby Cluster around PKS 1353−341". The Astrophysical Journal. 863 (2): 122. arXiv:1806.05676. Bibcode:2018ApJ...863..122S. doi:10.3847/1538-4357/aace55. eISSN 1538-4357.
  5. ^ Véron-Cetty, M.-P.; Véron, P. (July 2010). "A catalogue of quasars and active nuclei: 13th edition". Astronomy & Astrophysics. 518: A10. Bibcode:2010A&A...518A..10V. doi:10.1051/0004-6361/201014188. eISSN 1432-0746. ISSN 0004-6361.
  6. ^ Flesch, Eric W. (2015). "The Half Million Quasars (HMQ) Catalogue". Publications of the Astronomical Society of Australia. 32. arXiv:1502.06303. Bibcode:2015PASA...32...10F. doi:10.1017/pasa.2015.10. eISSN 1448-6083. ISSN 1323-3580.
  7. ^ a b Véron-Cetty, M. -P.; Woltjer, L.; Staveley-Smith, L.; Ekers, R. D. (October 2000). "The nature of powerful compact radio galaxies". Astronomy and Astrophysics. 362: 426–434. Bibcode:2000A&A...362..426V. ISSN 0004-6361.
  8. ^ a b Massaro, E.; Maselli, A.; Leto, C.; Marchegiani, P.; Perri, M.; Giommi, P.; Piranomonte, S. (18 April 2015). "The 5th edition of the Roma-BZCAT. A short presentation". Astrophysics and Space Science. 357 (1): 75. arXiv:1502.07755. Bibcode:2015Ap&SS.357...75M. doi:10.1007/s10509-015-2254-2. eISSN 1572-946X. ISSN 0004-640X. S2CID 254255813.
  9. ^ Skrutskie, M. F.; Cutri, R. M.; Stiening, R.; Weinberg, M. D.; Schneider, S.; Carpenter, J. M.; Beichman, C.; Capps, R.; Chester, T.; Elias, J.; Huchra, J.; Liebert, J.; Lonsdale, C.; Monet, D. G.; Price, S.; Seitzer, P.; Jarrett, T.; Kirkpatrick, J. D.; Gizis, J. E.; Howard, E.; Evans, T.; Fowler, J.; Fullmer, L.; Hurt, R.; Light, R.; Kopan, E. L.; Marsh, K. A.; McCallon, H. L.; Tam, R.; Van Dyk, S.; Wheelock, S. (February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. eISSN 1538-3881. ISSN 0004-6256.
  10. ^ "PKS 1353-341". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2024-11-11.
  11. ^ Preston, R. A.; Morabito, D. D.; Williams, J. G.; Faulkner, J.; Jauncey, D. L.; Nicolson, G. (September 1985). "A VLBI survey at 2.29 GHz". The Astronomical Journal. 90: 1599. Bibcode:1985AJ.....90.1599P. doi:10.1086/113869. ISSN 0004-6256.
  12. ^ Siebert, J.; Brinkmann, W.; Drinkwater, M. J.; Yuan, W.; Francis, P. J.; Peterson, B. A.; Webster, R. L. (November 1998). "X-ray properties of the Parkes sample of flat-spectrum radio sources: dust in radio-loud quasars?". Monthly Notices of the Royal Astronomical Society. 301 (1): 261–279. arXiv:astro-ph/9808065. Bibcode:1998MNRAS.301..261S. doi:10.1046/j.1365-8711.1998.02019.x. eISSN 1365-2966. ISSN 0035-8711.
  13. ^ Arce, Nicole. "Dazzling Galaxy Cluster Hiding In Plain Sight In Milky Way Neighborhood". Tech Times. Retrieved July 26, 2018.
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