NGC 526
The topic of NGC 526 has been the subject of much debate and controversy in recent years. Since its appearance, it has captured the attention of experts and fans alike, generating endless opinions and points of view. In this article, we will explore in depth the most relevant aspects related to NGC 526, analyzing its origins, evolution and its impact on current society. Likewise, we will examine the various perspectives that exist around this topic, providing a broad and complete vision that allows the reader to understand its complexity.
| NGC 526 | |
|---|---|
 legacy surveys image of NGC 526 | |
| Observation data (J2000 epoch) | |
| Constellation | Sculptor |
| Right ascension | 01h 23m 58.5s[1] |
| Declination | −35° 07′ 21″[1] |
| Redshift | 0.019220 [1] |
| Heliocentric radial velocity | 5762 km/h [1] |
| Galactocentric velocity | 5713 km/h [1] |
| Distance | 91.4 ± 6.4 Mpc (298.1 ± 18.0 Mly) [1] |
| Apparent magnitude (V) | 14.71 [1] |
| Characteristics | |
| Type | S0? [1] |
| Apparent size (V) | 1.6' x 0.3' [2] |
| Other designations | |
| ESO 352-IG 066, ESO 012138-3519.7, PGC 5120 [1] | |
NGC 526 is a pair of interacting lenticular galaxies in the constellation of Sculptor. Both the constituents are classified as S0 lenticular galaxies. This pair was first discovered by John Herschel on September 1, 1834. Dreyer, the compiler of the catalogue described the galaxy as "faint, small, a little extended, the preceding of 2", the other object being NGC 527.
See also
References
External links
Media related to NGC 526 at Wikimedia Commons- NGC 526 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- SEDS
