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NGC 3726

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NGC3726
CometC/2012 K1passing near NGC 3726.NEOWISEseries ofinfraredimages.
Observation data (J2000epoch)
ConstellationUrsa Major
Right ascension11h33m21.1s[1]
Declination47° 01′ 45″[1]
Redshift866 ± 1km/s[1]
Distance46.6± 11.2Mly(14.3 ± 3.4Mpc)[1]
Apparent magnitude(V)10.2
Characteristics
TypeSAB(r)c[1]
Apparent size(V)6.2× 4.3[1]
Other designations
UGC6537,MCG+08-21-051,PGC35676[1]

NGC 3726is abarredspiral galaxylocated in the constellationUrsa Major.It is located at a distance of circa 45 millionlight yearsfrom Earth, which, given its apparent dimensions, means that NGC 3726 is about 85,000 light years across. It was discovered byWilliam Herschelon February 5, 1788.[2]

Structure

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NGC 3726 is a spiral galaxy with a smallbar,seen with medium inclination.[3]The bar is 1.38 arcseconds across and it ends at an inner ring with 1.50 arcseconds diameter.[4]The bluest regions of star formation are located at the ring.[5]

Three arms emanate from the ring. The southern is the brightest and the north is the best defined. The third arm emanates from the east side of the ring, moves towards NNW and then bends sharply to the southwest.[6]Thespiral armsare thick and well defined and can be traced for half a revolution. The arms then branch into fragments. The spiral pattern of the galaxy is a bit disturbed[7]and asymmetrical.[6]Numerous brightHII regionsare present in the galaxy.[7]The galaxy has a massivedark matterhalo.[5]

The nucleus of the galaxy hosts asupermassive black holewith mass 106.5(3 million)M,based onKsbulge luminosity.[8]

Nearby galaxies

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NGC 3726 belongs in theNGC 3877group,[9]which is part of the southUrsa Major groups,part of theVirgo Supercluster.[10]Other galaxies in the same group areNGC 3893,NGC 3896,NGC 3906,NGC 3928,NGC 3949,NGC 3985,andNGC 4010.[9]It may be also kinematically related with the smaller galaxiesNGC 3769andNGC 3782,located at angular distances 68' and 69' respectively.[7]

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References

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  1. ^abcdefg"NASA/IPAC Extragalactic Database".Results for NGC 3726.Retrieved2016-01-18.
  2. ^NGC 3726cseligman.com
  3. ^Möllenhoff, C.; Heidt, J. (15 March 2001)."Surface photometry of spiral galaxies in NIR:Structural parameters of disks and bulges".Astronomy & Astrophysics.368(1): 16–37.Bibcode:2001A&A...368...16M.doi:10.1051/0004-6361:20000335.
  4. ^Comerón, S.; Salo, H.; Laurikainen, E.; Knapen, J. H.; Buta, R. J.; Herrera-Endoqui, M.; Laine, J.; Holwerda, B. W.; Sheth, K.; Regan, M. W.; Hinz, J. L.; Muñoz-Mateos, J. C.; Gil de Paz, A.; Menéndez-Delmestre, K.; Seibert, M.; Mizusawa, T.; Kim, T.; Erroz-Ferrer, S.; Gadotti, D. A.;Athanassoula, E.;Bosma, A.; Ho, L. C. (19 February 2014). "ARRAKIS: atlas of resonance rings as known in the S4G".Astronomy & Astrophysics.562:A121.arXiv:1312.0866.Bibcode:2014A&A...562A.121C.doi:10.1051/0004-6361/201321633.S2CID119295831.
  5. ^abGusev, A. S.; Zasov, A. V.; Kaisin, S. S.; Bizyaev, D. V. (September 2002). "BVRI surface photometry of the galaxy NGC 3726".Astronomy Reports.46(9): 704–711.Bibcode:2002ARep...46..704G.doi:10.1134/1.1508062.S2CID120372767.
  6. ^abEskridge, Paul B.; Frogel, Jay A.; Pogge, Richard W.; Quillen, Alice C.; Berlind, Andreas A.; Davies, Roger L.; DePoy, D. L.; Gilbert, Karoline M.; Houdashelt, Mark L.; Kuchinski, Leslie E.; Ramirez, Solange V.; Sellgren, K.; Stutz, Amelia; Terndrup, Donald M.; Tiede, Glenn P. (November 2002). "Near-Infrared and Optical Morphology of Spiral Galaxies".The Astrophysical Journal Supplement Series.143(1): 73–111.arXiv:astro-ph/0206320.Bibcode:2002ApJS..143...73E.doi:10.1086/342340.S2CID15491635.
  7. ^abcSandage, A., Bedke, J. (1994)The Carnegie Atlas of Galaxies. Volume I,Carnegie Institution of Washington
  8. ^Dong, X. Y.; De Robertis, M. M. (March 2006). "Low-Luminosity Active Galaxies and Their Central Black Holes".The Astronomical Journal.131(3): 1236–1252.arXiv:astro-ph/0510694.Bibcode:2006AJ....131.1236D.doi:10.1086/499334.S2CID17630682.
  9. ^abMakarov, Dmitry; Karachentsev, Igor (21 April 2011)."Galaxy groups and clouds in the local (z~ 0.01) Universe".Monthly Notices of the Royal Astronomical Society.412(4): 2498–2520.arXiv:1011.6277.Bibcode:2011MNRAS.412.2498M.doi:10.1111/j.1365-2966.2010.18071.x.S2CID119194025.Archived fromthe originalon 31 January 2016.Retrieved18 October2017.{{cite journal}}:CS1 maint: unflagged free DOI (link)
  10. ^"The Ursa Major Groups".www.atlasoftheuniverse.com.
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