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NGC 6008
NGC 6008 (sometimes referred to as NGC 6008A) is a barred spiral galaxy in the constellation of Serpens. Its velocity with respect to the cosmic microwave background is 4,959 ± 8 km/s, which corresponds to a Hubble distance of 73.2 ± 5.1 Mpc (~239 million light-years). It was discovered by French astronomer Édouard Stephan on 10 June 1880.
According to the SIMBAD database, NGC 6008 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
One supernova has been observed in NGC 6008:
According to A.M. Garcia, NGC 6008 is part of the NGC 6052 group (also known as LGG 403). This group has at least 13 members: NGC 5975, NGC 6020, NGC 6030, NGC 6032, NGC 6052, NGC 6060, NGC 6073, IC 1132, PGC 57117, UGC 10127, UGC 10197, and UGC 102116.
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NGC 6008
NGC 6008 (sometimes referred to as NGC 6008A) is a barred spiral galaxy in the constellation of Serpens. Its velocity with respect to the cosmic microwave background is 4,959 ± 8 km/s, which corresponds to a Hubble distance of 73.2 ± 5.1 Mpc (~239 million light-years). It was discovered by French astronomer Édouard Stephan on 10 June 1880.
According to the SIMBAD database, NGC 6008 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.
One supernova has been observed in NGC 6008:
According to A.M. Garcia, NGC 6008 is part of the NGC 6052 group (also known as LGG 403). This group has at least 13 members: NGC 5975, NGC 6020, NGC 6030, NGC 6032, NGC 6052, NGC 6060, NGC 6073, IC 1132, PGC 57117, UGC 10127, UGC 10197, and UGC 102116.