NGC 6627 is a barred spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 5,146±9 km/s, which corresponds to a Hubble distance of 247.6 ± 17.3 Mly (75.90 ± 5.31 Mpc). However, 25 non-redshift measurements give a much closer mean distance of 197.10 ± 15.05 Mly (60.432 ± 4.615 Mpc). It was discovered by German astronomer Albert Marth on 13 July 1863. NGC 6627 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 Three supernovae have been observed in NGC 6627:
SN 1998V (Type Ia, mag. 16) was discovered by British amateur astronomer Mark Armstrong on 10 March 1998. SN 2018evy (Type II, mag. 17.503) was discovered by ATLAS on 11 August 2018. SN 2021abkm (Type II, mag. 18.151) was discovered by ATLAS on 14 October 2021.
See also List of NGC objects (6001–7000)
References
External links NGC 6627 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images


