NGC 7606 is aspiral galaxy located in the constellationAquarius. It is located at a distance of circa 100 millionlight years from Earth, which, given its apparent dimensions, means that NGC 7606 is about 165,000 light years across. It was discovered byWilliam Herschel on September 28, 1785.[3] The galaxy is included in theHerschel 400 Catalogue. It lies 45 arcminutes northeast frompsi2 Aquarii. It can be seen with a 4 inchtelescope but its visibility is greatly affected bylight pollution.[4]
NGC 7606 is a spiral galaxy seen on inclination. It has a bright nucleus surrounded by a prominent bulge, which is seen elliptical due to the inclination. Nobar has been observed.[5] A ring with an apparent diameter of 0.85 arcminutes has been detected at the central part of the galaxy.[6] The galaxy features two main arms, that can be traced for nearly 360°, and several arm fragments.[5] The arms are smooth and rather tight, although not as tightly wound as the ones ofNGC 488.[7] Few bright spots have been observed in the arms.[5] The galaxy is found to host asupermassive black hole, whose mass based on bulge velocity dispersion σ is estimated to be 15-22 millionM☉.[8][9] NGC 7606 is an isolated galaxy.[10]
^abcEskridge, 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.
^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.
^Sandage, A., Bedke, J. (1994),The Carnegie Atlas of Galaxies. Volume I, Carnegie Institution of Washington
^Berrier, Joel C.; Davis, Benjamin L.; Kennefick, Daniel; Kennefick, Julia D.; Seigar, Marc S.; Barrows, Robert Scott; Hartley, Matthew; Shields, Doug; Bentz, Misty C.; Lacy, Claud H. S. (14 May 2013). "Further Evidence for a Supermassive Black Hole Mass-Pitch Angle Relation".The Astrophysical Journal.769 (2): 132.arXiv:1304.4937.Bibcode:2013ApJ...769..132B.doi:10.1088/0004-637X/769/2/132.S2CID118572496.
^Gingerich, Owen (1 November 1965)."Circular No. 1934".Central Bureau for Astronomical Telegrams. Smithsonian Astrophysical Observatory. Retrieved1 December 2024.
^"SN1965M".Transient Name Server.IAU. Retrieved1 December 2024.
^McNaught, R. H.; Evans, R.; Cragg, T.; Lee, S.; MacKie, G. (1987). "Supernova 1987N in NGC 7606".International Astronomical Union Circular (4511): 1.Bibcode:1987IAUC.4511....1M.
^"SN1987N".Transient Name Server.IAU. Retrieved1 December 2024.
^List of SupernovaeIAU Central Bureau for Astronomical Telegrams. Retrieved 29 December 2015.
