TXS 1321+045
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| TXS 1321+045 | |
|---|---|
 TXS 1321+045 captured with DESI Legacy Surveys | |
| Observation data (J2000.0 epoch) | |
| Constellation | Virgo |
| Right ascension | 13h 24m 19.67s[1] |
| Declination | +04° 19′ 07.20″[1] |
| Redshift | 0.263061[1] |
| Heliocentric radial velocity | 78,864 km/s[1] |
| Distance | 3.177 Gly |
| Group or cluster | MaxBCG J201.08197+04.31863 |
| Apparent magnitude (B) | 19.5 |
| Characteristics | |
| Type | BrCLG AGN[1] |
| Size | ~635,000 ly (194.6 kpc) (estimated)[1] |
| Other designations | |
| 2MASX J13241962+0419068, 1321+045, OGC 627, NVSS J132419+041906, RX J1324.2+0419, MaxBCG J201.08197+04.31863 BCG, RGB J1324+043[1] LEDA 3807422 | |
TXS 1321+045 or 1321+045, is a radio galaxy located in the constellation of Virgo. The redshift of the galaxy is (z) 0.263[1][2] and it was first discovered as a radio-loud object from the Sloan Digital Sky Survey (SDSS).[3] This object is classified as the brightest cluster galaxy (BCG) of the galaxy cluster, MaxBCG J201.08197+04.31863 and as such dominates the cluster. It also contains a compact steep spectrum source (CSS).[4][5][6]
TXS 1321+045 is categorized as a low-excitation radio galaxy (LERG) of low luminosity.[7][8][9] The structure of the galaxy is found to be compact based on high resolution imaging made with MERLIN, comprising at least three components; mainly a central radio core and two radio lobes that are found on the opposite sides of the core. The total flux density of the core is estimated to be 11 ± 2 mJy, while the lobes have flux densities of 38 ± 4 and 49 ± 5 mJy.[4] Observations made by MERLIN at 1.6 GHz frequencies have detected the same core with diffused radio emission from opposite sides.[2] Further observations have also shown the source is extended by around 40 kiloparsecs,with two knot features that are embedded inside an extended region.[10]
Observations made by the Very Long Baseline Interferometry (VLBI) at both 4.5 and 7.5 GHz frequencies have found the core is divided into two separate components, with total measured flux densities of 1.24 ± 0.03 and 0.74 ± 0.44 mJy. The secondary component is classified as a radio jet that has a linear size of around 20 parsecs. However its orientation degree is different compared to the lobes, indicating a new activity phase has begun recently with the fact the outer parts of the lobes are no longer evolving.[4]
The central supermassive black hole of the galaxy is estimated to be 9.46 ± 1.42 M☉ based on the study of compact sources published in 2025. The stellar velocity dispersion is estimated to be 333.13 ± 49.97 kilometers per seconds.[11] A study published in 2013, found the galaxy is undergoing star formation of 5.38 M☉ per year.[12]
References
- 1 2 3 4 5 6 7 8 "NED Search results for TXS 1321+045". NASA/IPAC Extragalactic Database. Retrieved 2026-01-15.
- 1 2 Kunert-Bajraszewska, M.; Gawroński, M. P.; Labiano, A.; Siemiginowska, A. (November 2010). "A survey of low-luminosity compact sources and its implication for the evolution of radio-loud active galactic nuclei - I. Radio data". Monthly Notices of the Royal Astronomical Society. 408 (4): 2261–2278. arXiv:1009.5235. Bibcode:2010MNRAS.408.2261K. doi:10.1111/j.1365-2966.2010.17271.x. ISSN 0035-8711.
- ↑ Best, P. N.; Kauffmann, G.; Heckman, T. M.; Ivezić, Ž (September 2005). "A sample of radio-loud active galactic nuclei in the Sloan Digital Sky Survey". Monthly Notices of the Royal Astronomical Society. 362 (1): 9–24. arXiv:astro-ph/0506268. Bibcode:2005MNRAS.362....9B. doi:10.1111/j.1365-2966.2005.09283.x. ISSN 0035-8711.
- 1 2 3 O’Sullivan, Ewan; Kunert-Bajraszewska, Magdalena; Siemiginowska, Aneta; Burke, D. J.; Combes, Françoise; Salomé, Philippe; Giacintucci, Simona (2021-06-01). "The Cluster-central Compact Steep-spectrum Radio Galaxy 1321+045". The Astrophysical Journal. 913 (2): 105. arXiv:2104.04548. Bibcode:2021ApJ...913..105O. doi:10.3847/1538-4357/abf6c6. ISSN 0004-637X.
- ↑ O'Sullivan, Ewan; Kunert-Bajraszewska, Magdalena; Siemiginowska, Aneta; Burke, Douglas J.; Combes, Françoise; Salomé, Philippe; Giacintucci, Simona (2021). "1321+045: A compact steep-spectrum radio source in a cool-core galaxy cluster". Astronomische Nachrichten. 342 (9–10): 1155–1159. doi:10.1002/asna.20210035. ISSN 1521-3994.
- ↑ Ubertosi, F.; Gitti, M.; Brighenti, F.; Olivares, V.; O’Sullivan, E.; Schellenberger, G. (2023-05-01). "Waking the monster: The onset of AGN feedback in galaxy clusters hosting young central radio galaxies". Astronomy & Astrophysics. 673: A52. arXiv:2303.04821. Bibcode:2023A&A...673A..52U. doi:10.1051/0004-6361/202345894. ISSN 0004-6361.
- ↑ Meusinger, H.; Mhaskey, M. (2023-11-25), "A comparison of compact, presumably young with extended, evolved radio active galactic nuclei", Astronomy and Astrophysics, 682: A18, arXiv:2311.15009, Bibcode:2024A&A...682A..18M, doi:10.1051/0004-6361/202243388, retrieved 2026-01-15
- ↑ Kunert-Bajraszewska, M.; Labiano, A.; Siemiginowska, A.; Guainazzi, M. (February 2014). "First X-ray observations of low-power compact steep spectrum sources". Monthly Notices of the Royal Astronomical Society. 437 (4): 3063–3071. arXiv:1311.6633. doi:10.1093/mnras/stt1978. ISSN 0035-8711.
- ↑ Kunert-Bajraszewska, M.; Siemiginowska, A.; Labiano, A. (2013-07-05). "An X-Ray Cooling-Core Cluster Surrounding a Low-Power Compact Steep Spectrum Radio Source 1321+045". The Astrophysical Journal. 772 (1): L7. arXiv:1306.5579. Bibcode:2013ApJ...772L...7K. doi:10.1088/2041-8205/772/1/l7. ISSN 2041-8205.
- ↑ Kunert-Bajraszewska, M.; Labiano, A. (2010-09-27), "A survey of low-luminosity compact sources and its implication for the evolution of radio-loud active galactic nuclei - II. Optical analysis", Monthly Notices of the Royal Astronomical Society, 408 (4): 2279–2289, arXiv:1009.5237, Bibcode:2010MNRAS.408.2279K, doi:10.1111/j.1365-2966.2010.17300.x
- ↑ Marques, Bárbara L. Miranda; Rodríguez-Ardila, Alberto; Fonseca-Faria, Marcos A.; Panda, Swayamtrupta (2024-11-18), "Powerful outflows of compact radio galaxies", The Astrophysical Journal, 978 (1): 16, arXiv:2411.03130, Bibcode:2025ApJ...978...16M, doi:10.3847/1538-4357/ad8f40, retrieved 2026-01-15
- ↑ Liu, F. S.; Mao, Shude; Meng, X. M. (2012-03-08), "Star formation activities in early-type brightest cluster galaxies", Monthly Notices of the Royal Astronomical Society, 423 (1): 422–436, arXiv:1203.1840, Bibcode:2012MNRAS.423..422L, doi:10.1111/j.1365-2966.2012.20886.x
