ESO 291- G010, AM 2312-435, MCG -07-47-025, PGC 70800[1]
NGC 7531 is an intermediate spiral galaxy located in the constellation Grus. It is located at a distance of about 70 million light-years from Earth, which, given its apparent dimensions, means that NGC 7531 is about 95,000 light years across.[1] It was discovered by John Herschel on September 2, 1836.[2]
Characteristics
The inner region of NGC 7531 is characterized by a high surface brightness ring. The ring is a place of active star formation and a number of star clusters and H II regions have been identified in it.[3] The star formation rate of the inner ring is estimated to be 0.41 ± 0.12 M☉ per year based on H-alpha emission.[4] A weak bar is observed in the near infrared inside the ring, along with dust lanes. Yet, the motions at the inner ring are predominately circular. The inner ring may lie at the location of the inner Lindblad resonance.[3]
The galaxy has two patchy spiral arms that are relatively well defined but are of low surface brightness. H II regions have also been observed at the spiral arms of the galaxy, where there is also active star formation, which is more intense at the southwest region.[3] A supermassive black hole is believed to lie in the centre of the galaxy whose mass is estimated to be 3–48 million (107.07±0.61) M☉, based on the spiral arm pitch angle.[5] The galaxy is seen with an inclination of 66°.[3]
In long exposure photographic plates of the galaxy, a large low surface brightness region structure was observed 2.6 arcminutes west from the nucleus of the galaxy, that has more than half the apparent diameter of NGC 7531.[3] It has been identified as a stellar cloud that may be a dwarf satellite of the galaxy or a shell created by the tidal disruption of NGC 7531.[7]
12345Buta, R. (May 1987). "The structure and dynamics of ringed galaxies. III - Surface photometry and kinematics of the ringed nonbarred spiral NGC 7531". The Astrophysical Journal Supplement Series. 64: 1. Bibcode:1987ApJS...64....1B. doi:10.1086/191190.
↑Davis, Benjamin L.; Berrier, Joel C.; Johns, Lucas; Shields, Douglas W.; Hartley, Matthew T.; Kennefick, Daniel; Kennefick, Julia; Seigar, Marc S.; Lacy, Claud H. S. (20 June 2014). "The Black Hole Mass Function Derived from Local Spiral Galaxies". The Astrophysical Journal. 789 (2): 124. arXiv:1405.5876. Bibcode:2014ApJ...789..124D. doi:10.1088/0004-637X/789/2/124. S2CID119302157.
↑List of SupernovaeIAU Central Bureau for Astronomical Telegrams. Retrieved 29 December 2015.
↑Martínez-Delgado, David; Gabany, R. Jay; Crawford, Ken; Zibetti, Stefano; Majewski, Steven R.; Rix, Hans-Walter; Fliri, Jürgen; Carballo-Bello, Julio A.; Bardalez-Gagliuffi, Daniella C.; Peñarrubia, Jorge; Chonis, Taylor S.; Madore, Barry; Trujillo, Ignacio; Schirmer, Mischa; McDavid, David A. (1 October 2010). "Stellar tidal streams in spiral galaxies of the local volume: a pilot survey with modest aperture telescopes". The Astronomical Journal. 140 (4): 962–967. arXiv:1003.4860. Bibcode:2010AJ....140..962M. doi:10.1088/0004-6256/140/4/962. S2CID43034946.
