NGC 1418
| NGC 1418 | |
|---|---|
NGC 1418 imaged by Legacy Surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 42m 16.1773s[1] |
| Declination | −04° 43′ 51.406″[1] |
| Redshift | 0.014023±0.0000200[1] |
| Heliocentric radial velocity | 4,204±6 km/s[1] |
| Distance | 213.91 ± 26.41 Mly (65.586 ± 8.097 Mpc)[2] |
| Group or cluster | NGC 1417 group (LGG 103[3] |
| Apparent magnitude (V) | 14.21[1] |
| Characteristics | |
| Type | SB(s)b[1] |
| Size | ~100,800 ly (30.91 kpc) (estimated)[1] |
| Apparent size (V) | 1.3′ × 0.9′[1] |
| Other designations | |
| HOLM 70B, 2MASX J03421615-0443505, MCG -01-10-022, PGC 13606[1] | |
NGC 1418 is a barred spiral galaxy in the constellation of Eridanus. Its velocity with respect to the cosmic microwave background is 4,068±11 km/s, which corresponds to a Hubble distance of 195.7 ± 13.7 Mly (59.99 ± 4.20 Mpc).[1] However, seven non-redshift measurements give a farther mean distance of 213.91 ± 26.41 Mly (65.586 ± 8.097 Mpc).[2] It was discovered by German-British astronomer William Herschel on 5 October 1785.[4]
NGC 1418 has a possible active galactic nucleus, 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.[5][6]
NGC 1417 group
[edit]NGC 1418 is a member of the NGC 1417 galaxy group (also known as LGG 103). This group contains at least 14 galaxies, including NGC 1358, NGC 1376, NGC 1417, NGC 1441, NGC 1449, NGC 1451, and NGC 1453.[3][7]
Supernovae
[edit]Two supernovae has been observed in NGC 1418:
See also
[edit]References
[edit]- 1 2 3 4 5 6 7 8 9 10 "Results for object NGC 1418". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved 4 September 2026.
- 1 2 "Distance Results for NGC 1418". NASA/IPAC Extragalactic Database. NASA. Retrieved 4 September 2026.
- 1 2 Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.
- ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 1418". Celestial Atlas. Retrieved 4 September 2026.
- ↑ Asmus, D.; Greenwell, C. L.; Gandhi, P.; Boorman, P. G.; Aird, J.; Alexander, D. M.; Assef, R. J.; Baldi, R. D.; Davies, R. I.; Hönig, S. F.; Ricci, C.; Rosario, D. J.; Salvato, M.; Shankar, F.; Stern, D. (2020). "Local AGN survey (LASr): I. Galaxy sample, infrared colour selection, and predictions for AGN within 100 MPC". Monthly Notices of the Royal Astronomical Society. 494 (2): 1784. arXiv:2003.05959. Bibcode:2020MNRAS.494.1784A. doi:10.1093/mnras/staa766.
- ↑ "NGC 1418". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 4 September 2026.
- ↑ "LGG 103". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 4 September 2026.
- ↑ Kim, H.; Zheng, W.; Li, W.; et al. (2013). "Supernova 2013gy in NGC 1418 = PSN J03421688-0443185". Central Bureau Electronic Telegrams (3743): 1. Bibcode:2013CBET.3743....1K.
- ↑ "SN 2013gy". Transient Name Server. IAU. Retrieved 4 September 2026.
- ↑ "SN 2026aadx". Transient Name Server. IAU. Retrieved 4 September 2026.
External links
[edit]
Media related to NGC 1418 at Wikimedia Commons- NGC 1418 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images