| UGC 11105 | |
|---|---|
.jpg) Hubble Space Telescope image of UGC 11105 | |
| Observation data (J2000 epoch) | |
| Constellation | Hercules |
| Right ascension | 18 04 36.08 |
| Declination | +21° 38′ 16.2″ |
| Redshift | 0.007418 |
| Heliocentric radial velocity | 2216 ± 4 km/s |
| Distance | 109 Mly (33.4 Mpc) |
| Apparent magnitude (B) | 15.7 |
| Characteristics | |
| Type | Sdm |
| Size | ~81,100 ly (24.87 kpc) (estimated) |
| Other designations | |
| PGC 61361, UGC 11105, MCG +04-42-024, CGCG 141-047 | |
UGC 11105, also known as PGC 61361, is a relatively nearby spiral galaxy located 109 million light-years (33.4 Mpc) away in the Hercules constellation. The galaxy is outshone by bright stars in the foreground. From the perspective on Earth, the Sun is 14 thousand trillion times brighter as compared to UGC 1105, if we to calculate the apparent magnitude for both objects. It is a possible active galactic nucleus candidate, according to SIMBAD.
One supernova has been observed in UGC 11105: SN 2019pjs (type II, mag. 17.3).
References
- ^ "UGC 11105". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2024-10-30.
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-04-20.
- ^ information@eso.org. "Dim, but still distinct". esahubble.org. Retrieved 2024-04-20.
- Transient Name Server entry for SN 2019pjs. Retrieved 27 July 2024.
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