NGC 7237

Last updated
NGC 7237
NGC7237 - SDSS DR14.jpg
NGC 7237 by PanSTARRS
Observation data (J2000 epoch)
Constellation Pegasus
Right ascension 22h 14m 46.9s [1]
Declination +13° 50′ 27″ [1]
Redshift 0.026213 ± 0.000007 [1]
Helio radial velocity 7,858 ± 2 km/s [1]
Distance 371 ± 99 Mly (114 ± 30.5 Mpc) [1]
Apparent magnitude  (V)13.9 [2]
Characteristics
Type SA0- [1]
Apparent size  (V)1.81′ × 0.72′ [1]
Notable featuresInteracting galaxy, radio galaxy
Other designations
UGC 11958, Arp 169, II Zw 172, CGCG 428-058, MCG +02-56-024, 3C 442A, PGC 68383 [1]

NGC 7237 is an interacting lenticular galaxy located in the constellation Pegasus. It is located at a distance of about 350 million light years from Earth, which, given its apparent dimensions, means that NGC 7237 is about 240,000 light years across. [1] NGC 7237 forms a pair with NGC 7236 and is a radio galaxy. It was discovered by Albert Marth on August 25, 1864. [3]

Contents

NGC 7237 forms a pair with lenticular galaxy NGC 7236, [4] which lies 35 arcseconds to the northwest. The two galaxies are undergoing a merger and are surrounded by hot gas (corona) with temperature of around 1 keV. The total mass of that gas is estimated to be 3×1010  M☉ . [5] A smaller elliptical galaxy, NGC 7237C, lies 38 arcseconds southeast of NGC 7237. It is included in the Atlas of Peculiar Galaxies , in the category diffuse counter-tails. A tail is also visible in X-rays. [6] The isophotes in the central region of NGC 7237 are irregular. [7]

The galaxy pair is a source of radiowaves. The radio emission has a double lobe structure, with filaments, but no jets, while a weak core is identified as the nucleus of NGC 7237. [8] The filaments could be created by the interaction of hot gas with the preexisting radio emitting plasma. Some bright radio sources are visible within the lobes but they could be background active galaxies. [6] The core has been found to be variable source of X-rays. [6]

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<span class="mw-page-title-main">NGC 547</span> Galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 1142</span> Interacting and distorted spiral galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 5252</span> Galaxy in the constellation of Virgo

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<span class="mw-page-title-main">NGC 2110</span>

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<span class="mw-page-title-main">NGC 7720</span>

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<span class="mw-page-title-main">NGC 5532</span> Galaxy in the constellation of Virgo

NGC 5532 is an elliptical galaxy located in the constellation Boötes. It is located at a distance of about 250 million light years from Earth, which, given its apparent dimensions, means that NGC 5532 is about 110,000 light years across. It was discovered by William Herschel on March 15, 1784. It is a Fanaroff–Riley type 1 (FR1) radio galaxy.

<span class="mw-page-title-main">NGC 7236</span>

NGC 7236 is an interacting lenticular galaxy located in the constellation Pegasus. It is located at a distance of about 300 million light years from Earth, which, given its apparent dimensions, means that NGC 7236 is about 150,000 light years across. NGC 7236 forms a pair with NGC 7237 and is a radio galaxy. It was discovered by Albert Marth on August 25, 1864.

<span class="mw-page-title-main">NGC 3801</span>

NGC 3801 is a lenticular galaxy located in the constellation Leo. It is about 150 million light years from Earth, and estimated to be about 170,000 light years in diameter. William Herschel discovered it on 17 April 1784.

References

  1. 1 2 3 4 5 6 7 8 9 "NASA/IPAC Extragalactic Database". Results for NGC 7237. Retrieved 2023-07-07.
  2. ↑ "Revised NGC Data for NGC 7237". spider.seds.org. Retrieved 25 November 2018.
  3. ↑ Seligman, Courtney. "NGC 7237 (with NGC 7236 = Arp 169)". Celestial Atlas. Retrieved 19 November 2018.
  4. ↑ Borne, Kirk D.; Hoessel, John G. (July 1988). "Interacting binary galaxies. III - Observations of NGC 1587/1588 and NGC 7236/7237". The Astrophysical Journal. 330: 51. doi:10.1086/166454.
  5. ↑ Worrall, D. M.; Birkinshaw, M.; Kraft, R. P.; Hardcastle, M. J. (1 April 2007). "The Effect of a Chandra -measured Merger-related Gas Component on the Lobes of a Dead Radio Galaxy". The Astrophysical Journal. 658 (2): L79–L82. doi: 10.1086/513869 . S2CID   15963632.
  6. 1 2 3 Hardcastle, M. J.; Kraft, R. P.; Worrall, D. M.; Croston, J. H.; Evans, D. A.; Birkinshaw, M.; Murray, S. S. (10 June 2007). "The Interaction between Radio Lobes and Hot Gas in the Nearby Radio Galaxies 3C 285 and 3C 442A". The Astrophysical Journal. 662 (1): 166–181. arXiv: astro-ph/0703080 . doi:10.1086/517997. S2CID   18803836.
  7. ↑ Martel, André R.; Baum, Stefi A.; Sparks, William B.; Wyckoff, Eric; Biretta, John A.; Golombek, Daniel; Macchetto, Ferdinando D.; de Koff, Sigrid; McCarthy, Patrick J.; Miley, George K. (May 1999). "Hubble Space Telescope Snapshot Survey of 3CR Radio Source Counterparts. III. Radio Galaxies with [FORMULA][F]z". The Astrophysical Journal Supplement Series. 122 (1): 81–108. doi: 10.1086/313205 . S2CID   249153931.
  8. ↑ Comins, Neil F.; Owen, Frazer N. (November 1991). "The extraordinary radio source 3C 442". The Astrophysical Journal. 382: 108. doi:10.1086/170698.
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