NGC 7537
Template:Short description Template:Infobox Galaxy
NGC 7537 is a spiral galaxy located in the equatorial constellation of Pisces, about 1.5° to the NNW of Gamma Piscium.[1] It was first documented by German-born astronomer William Herschel on Aug 30, 1785. J. L. E. Dreyer described it as, "very faint, considerably small, round, brighter middle, southwestern of 2".[2] This galaxy lies at a distance of approximately Script error: No such module "convert". from the Milky Way,[3] and is a member of the Pegasus I cluster.[4]
This object forms a pair with the nearly edge-on barred spiral galaxy NGC 7541, and the two show signs of interaction. NGC 7537 has a curved tidal tail to the northeast with a length of Script error: No such module "convert"., while NGC 7541 has two tidal tails. They have a projected separation of Script error: No such module "convert"..[5]
A Type II supernova[6] designated SN 2002gd was detected by multiple independent observers beginning October 5, 2002. It was positioned Script error: No such module "val". east and Script error: No such module "val". north of the galactic nucleus of NGC 7537.[7]
References
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