3C 132
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| 3C 132 | |
|---|---|
 SDSS image of 3C 132 | |
| Observation data (J2000.0 epoch) | |
| Constellation | Taurus |
| Right ascension | 04h 56m 43.01s[1] |
| Declination | +22° 49′ 22.95″[1] |
| Redshift | 0.214000[1] |
| Heliocentric radial velocity | 64,156 km/s[1] |
| Distance | 2.661 Gly |
| Apparent magnitude (B) | 18.5 |
| Characteristics | |
| Type | Radio galaxy LEG[1] |
| Size | ~344,000 ly (105.46 kpc) (estimated)[1] |
| Other designations | |
| 4C +22.11, PKS 0453+22, LEDA 2817548, B2 0453+22, 2MASX J04564292+2249230, NRAO 0198, NVSS J045643+224922, Cul 0453+227, G4Jy 0511[1] | |
3C 132 is a radio galaxy located in the constellation of Taurus. The redshift of the galaxy is (z) 0.214[1] and it was first discovered in the Third Cambridge Catalogue of Radio Sources survey in 1962.[2] The source of the galaxy is known to display evidence of lunar occultations.[3]
3C 132 is classified as a Fanaroff-Riley class Type 2 low-excitation radio galaxy.[4] The host galaxy is an elliptical galaxy with a smooth and elongated appearance, but is also described as an interacting irregular galaxy[5][6] The galaxy is also surrounded by several companions forming a packed group, suggesting it also resides inside a galaxy cluster.[5][7] A face-on disk is found in the galaxy described to have an elliptical isotphotal morphology.[8] Imaging made by Hubble Space Telescope (HST) found a bright central nucleus.[9] This nucleus is described as being surrounded by faint diffused radio emission.[10]
The radio source of the galaxy is a classical double, with two components having a flux ratio of 1.6 ± 0.3.[11] When observed at high resolutions with the Very Large Array (VLA) it has hotspot regions protruding in a bottle-neck fashion, with brightening observed in its radio lobe located on the eastern side, just along the southern edge. The hotspot on the western side is 800 parsecs in extent .while the eastern one is estimated to be 2 kiloparsecs. A curved feature interpreted as backflow is leaving the location of the western hotspot towards the southeast. Upon reaching seven kiloparsecs from the hotspot, a bend is observed in the feature before subsequently ending inside a region of diffused medium.[12] There is also a radio bridge present in the source, perpendicular towards its axis.[13]
A study in 2014 showed the edge-brightened lobes of the galaxy on the southwest and northwestern sides have the same brightness. Upon observation, the lobes are shown flaring towards the direction of the core. A knot feature described as faint is located inside the southeastern lobe, apparently bridging a delineated section and a diffused region.[14]
References
- 1 2 3 4 5 6 7 8 "NED Search results for 3C 132". NASA/IPAC Extragalactic Database. Retrieved 2025-09-27.
- ↑ Bennett, A. S. (1962). "The revised 3C catalogue of radio sources". Memoirs of the Royal Astronomical Society. 68: 163. Bibcode:1962MmRAS..68..163B.
- ↑ Taylor, J. H. (December 1966). "Lunar Occultations of Five Radio Sources". The Astrophysical Journal. 146: 646. Bibcode:1966ApJ...146..646T. doi:10.1086/148942. ISSN 0004-637X.
- ↑ Massaro, F.; Harris, D. E.; Tremblay, G. R.; Axon, D.; Baum, S. A.; Capetti, A.; Chiaberge, M.; Gilli, R.; Giovannini, G.; Grandi, P.; Macchetto, F. D.; O’Dea, C. P.; Risaliti, G.; Sparks, W. (2010-04-13). "CHANDRAOBSERVATIONS OF 3C RADIO SOURCES WITHz< 0.3: NUCLEI, DIFFUSE EMISSION, JETS, AND HOTSPOTS". The Astrophysical Journal. 714 (1): 589–604. arXiv:1003.2438. Bibcode:2010ApJ...714..589M. doi:10.1088/0004-637x/714/1/589. ISSN 0004-637X.
- 1 2 Floyd, David J. E.; Axon, David; Baum, Stefi; Capetti, Alessandro; Chiaberge, Marco; Macchetto, Duccio; Madrid, Juan; Miley, George; O’Dea, Christopher P.; Perlman, Eric; Quillen, Alice; Sparks, William; Tremblay, Grant (July 2008). "Hubble Space TelescopeNear-infrared Snapshot Survey of 3CR Radio Source Counterparts. II. An Atlas and Inventory of the Host Galaxies, Mergers, and Companions". The Astrophysical Journal Supplement Series. 177 (1): 148–173. arXiv:0712.0595. Bibcode:2008ApJS..177..148F. doi:10.1086/587622. ISSN 0067-0049.
- ↑ Hutchings, J. B. (September 1987). "What is the difference between radio galaxies and radio quasar galaxies?". The Astrophysical Journal. 320: 122. Bibcode:1987ApJ...320..122H. doi:10.1086/165527. ISSN 0004-637X. Archived from the original on 2024-09-10.
- ↑ Hutchings, J. B.; Neff, S. G. (February 1997). "JHK Imaging and Photometry of Low Z QSOs and Radio Galaxy". The Astronomical Journal. 113: 550. arXiv:astro-ph/9611192. Bibcode:1997AJ....113..550H. doi:10.1086/118275. ISSN 0004-6256.
- ↑ Tremblay, G. R.; Chiaberge, M.; Donzelli, C. J.; Quillen, A. C.; Capetti, A.; Sparks, W. B.; Macchetto, F. D. (September 2007). "Isophotal Structure and Dust Distribution in Radio-loud Elliptical Galaxies". The Astrophysical Journal. 666 (1): 109–121. arXiv:0705.3642. Bibcode:2007ApJ...666..109T. doi:10.1086/520333. ISSN 0004-637X.
- ↑ de Koff, Sigrid; Baum, Stefi A.; Sparks, William B.; Biretta, John; Golombek, Daniel; Macchetto, Ferdinando; McCarthy, Patrick; Miley, George K. (December 1996). "HST Snapshot Survey of 3CR Radio Source Counterparts. I. Intermediate Redshifts". The Astrophysical Journal Supplement Series. 107 (2): 621–660. Bibcode:1996ApJS..107..621D. doi:10.1086/192376. ISSN 0067-0049.
- ↑ Tremblay, Grant R.; Chiaberge, Marco; Sparks, William B.; Baum, Stefi A.; Allen, Mark G.; Axon, David J.; Capetti, Alessandro; Floyd, David J. E.; Macchetto, F. Duccio; Miley, George K.; Noel-Storr, Jacob; O'Dea, Christopher P.; Perlman, Eric S.; Quillen, Alice C. (2009-07-23). "HST /ACS EMISSION LINE IMAGING OF LOW-REDSHIFT 3CR RADIO GALAXIES. I. THE DATA". The Astrophysical Journal Supplement Series. 183 (2): 278–294. arXiv:0906.4776. Bibcode:2009ApJS..183..278T. doi:10.1088/0067-0049/183/2/278. ISSN 0067-0049.
- ↑ Lyne, A. G. (1972-07-01). "A Study of the Lunar Occultations of Eleven Radio Sources" (PDF). Monthly Notices of the Royal Astronomical Society. 158 (4): 431–462. doi:10.1093/mnras/158.4.431. ISSN 0035-8711.
- ↑ Hardcastle, M. J.; Alexander, P.; Pooley, G. G.; Riley, J. M. (1997-07-11). "High-resolution observations at 3.6 cm of seventeen FR II radio galaxies with 0.15 <z< 0.30" (PDF). Monthly Notices of the Royal Astronomical Society. 288 (4): 859–890. doi:10.1093/mnras/288.4.859. ISSN 0035-8711.
- ↑ Gopal-Krishna (1977-11-01). "A study of the bridges in the radio galaxies 3C 132 and 3C 192 at metre and centimetre wavelengths". Monthly Notices of the Royal Astronomical Society. 181 (2): 247–252. doi:10.1093/mnras/181.2.247. ISSN 0035-8711.
- ↑ Fernini, Ilias (2014-05-15). "VERY LARGE ARRAY IMAGES AT 8.4 GHz OF 40 FANAROFF-RILEY II 3CR RADIO SOURCES WITH 0.1 < z < 2.0". The Astrophysical Journal Supplement Series. 212 (2): 19. Bibcode:2014ApJS..212...19F. doi:10.1088/0067-0049/212/2/19. ISSN 0067-0049.
External links
- 3C 132 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- 3C 132 on SIMBAD
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