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NGC 741

Summary

NGC 741, also known as PGC 7252, is a formerly active radio galaxy in the constellation of Pisces.[6][7][8] Located 74.13 Mpc away,[3] NGC 741 is part of a group of galaxies including NGC 742 and PGC 7250.[9] NGC 741 and NGC 742 recently collided, although the disruption was minor.[10] Radio filaments have been found connecting NGC 741 to NGC 742, and due to the bent structure of the radio filaments, NGC 741 is estimated to be moving at 1400 km/s with respect to its local group, suggesting that ram-pressure stripping was created as a product of the former merger.[11]

NGC 741
SDSS image of NGC 741
Observation data (J2000 epoch)
ConstellationPisces
Right ascension01h 56m 20.959s[1]
Declination+05° 37′ 43.77″[1]
Redshift0.01856[2]
Heliocentric radial velocity5513 km/s[2]
Distance241.8 Mly (74.13 Mpc)[3]
Group or clusterNGC 741 group[2]
Apparent magnitude (V)11.26[4]
Apparent magnitude (B)12.31[4]
Characteristics
TypeE0:[5]
Other designations
UGC 1413, MCG +01-06-003, PGC 7252[2]

References edit

  1. ^ a b Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi:10.1086/498708. ISSN 0004-6256. S2CID 18913331.
  2. ^ a b c d "NGC 741". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2021-02-12.
  3. ^ a b Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal. 655 (2): 790–813. arXiv:astro-ph/0610732. Bibcode:2007ApJ...655..790C. doi:10.1086/510201. S2CID 11672751.
  4. ^ a b "Search specification: NGC 741". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-12.
  5. ^ "Results for object NGC 0741 (NGC 741)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-12.
  6. ^ "Figure 1. Smoothed, exposure corrected Chandra images of NGC 741 in the..." ResearchGate. Retrieved 2019-05-25.
  7. ^ Jetha, Nazirah N.; Hardcastle, Martin J.; Babul, Arif; O'Sullivan, Ewan; Ponman, Trevor J.; Raychaudhury, Somak; Vrtilek, Jan (2008). "The nature of the ghost cavity in the NGC 741 group". Monthly Notices of the Royal Astronomical Society. 384 (4). Wiley-Blackwell: 1344–1354. arXiv:0712.1150. Bibcode:2008MNRAS.384.1344J. doi:10.1111/j.1365-2966.2007.12829.x. S2CID 15978368.
  8. ^ Jenkins, C. R.; Scheuer, P. A. G. (1980). "1980MNRAS.192..595J Page 595". Monthly Notices of the Royal Astronomical Society. 192. Cambridge, Massachusetts: Harvard University: 595. Bibcode:1980MNRAS.192..595J. doi:10.1093/mnras/192.4.595.
  9. ^ "New General Catalog Objects: NGC 700 - 749". cseligman.com. Retrieved 2019-05-19.
  10. ^ "Webb Deep-Sky Society: Galaxy of the Month: NGC741". www.webbdeepsky.com. Retrieved 2019-05-19.
  11. ^ Schellenberger, G.; Vrtilek, J.; David, L.; O'Sullivan, E.; Giacintucci, S.; Johnston-Hollitt, M.; Duchesne, S.; Raychaudhury, S. (2017-10-01). "NGC 741 - Mergers and AGN feedback on galaxy groups scale". The X-Ray Universe 2017: 205. Bibcode:2017xru..conf..205S.

External links edit

  •   Media related to NGC 741 at Wikimedia Commons