| NGC 428 | |
|---|---|
 Hubble image of NGC 428. | |
| Observation data (J2000.0epoch) | |
| Constellation | Cetus[1] |
| Right ascension | 01h 12m 55,709s[2] |
| Declination | +00° 58′ 53.69″[2] |
| Distance | 48mly[3] |
| Apparent magnitude (B) | 12.1[2] |
| Characteristics | |
| Type | SAB(s)m[4] |
| Other designations | |
| NGC 428 • UGC 763 • PGC 4367 • Z 385.28 • MCG + 00-04-36 • IRAS 01103 + 0043 • 2MASX J01125570 + 0058536 • GC 238 • H 2.622 • HIPASS J0112 + 00[2] | |
NGC 428 is abarred spiral galaxy in the constellation ofCetus (The Sea Monster), with its spiral structure distorted and warped, possibly the result of thecollision of two galaxies.[3] There appears to be a substantial amount ofstar formation occurring within NGC 428 and it lacks well defined arms — a telltale sign of a galaxy merger.[3] In 2015 theHubble Space Telescope made a close-up shot of the galaxy with itsAdvanced Camera for Surveys and itsWide Field and Planetary Camera 2.[1] The structure of NGC 428 has been compared toNGC 5645.[4]
NGC 428 was discovered byWilliam Herschel in December 1786.[3] Atype Ia supernova designatedSN2013ct was discovered May 11, 2013, within the galaxy by Stuart Parker of the Backyard Observatory Supernova Search (BOSS) project inAustralia andNew Zealand.[3][5]
Smoker et al. reported in 1996 on the NGC 428 field, with the HI tail andLSB dwarf 0110+008, assessingstar formation properties based on molecule density distributions, and concluded that the tail formation most likely originated throughtidal interactions between two galaxies.[6]
