NGC 6754 is a barred spiral galaxy in the constellation of Telescopium. Its velocity with respect to the cosmic microwave background is 3176 ± 11 km/s, which corresponds to a Hubble distance of 152.8 ± 10.7 Mly (46.84 ± 3.29 Mpc). Additionally, 10 non-redshift measurements give a closer distance of 137.15 ± 4.19 Mly (42.05 ± 1.285 Mpc). It was discovered by British astronomer John Herschel on 8 July 1834. According to the SIMBAD database, NGC 6754 is an Active Galaxy Nucleus Candidate, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars.
Supernovae Four supernovae have been observed in NGC 6754:
SN 1998X (Type II, mag. 17) was discovered by the Perth Astronomical Research Group on 13 March 1998. SN 1998dq (Type Ia, mag. 14.3) was discovered by Brett White on 23 August 1998. SN 2000do (Type Ia, mag. 15.6) was discovered by Brett White on 30 September 2000. SN 2005cu (Type II, mag. 16.1) was discovered by Berto Monard on 10 July 2005.
See also List of NGC objects (6001–7000)
References
External links Media related to NGC 6754 at Wikimedia Commons NGC 6754 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


