| UGC 711 | |
|---|---|
 | |
| Observation data (J2000 epoch) | |
| Constellation | Cetus |
| Right ascension | 01h 08m 36.90s |
| Declination | +01° 38′ 30.0″ |
| Redshift | 0.006611 |
| Heliocentric radial velocity | 1,982 km/s |
| Distance | 77 Mly (23.6 Mpc) |
| Apparent magnitude (V) | 0.069 |
| Apparent magnitude (B) | 0.092 |
| Surface brightness | 14.39 |
| Characteristics | |
| Type | SB (s)d?, sp |
| Apparent size (V) | 4.65' x 0.30' |
| Notable features | Superthin spiral galaxy |
| Other designations | |
| PGC 4063, FGC 0124, RFGC 0255, MCG +00-04-008, CGCG 385-005 | |
UGC 711 is a relatively nearby spiral galaxy located in the constellation of Cetus. Estimated to be located 77 million light-years from Earth,[1] the galaxy's luminosity class is IV and it has a HI line width region.[clarification needed][2] It belongs to the equatorial region of Eridanus Void with an arcsec approximation of ≈ 250.[clarification needed][3]
- ^ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2024-06-29.
- ^ Lu, N. Y.; Hoffman, G. L.; Groff, T.; Roos, T.; Lamphier, C. (1993-10-01). "H i 21 Centimeter Observations and I-Band CCD Surface Photometry of Spiral Galaxies behind the Virgo Cluster and toward Its Antipode". The Astrophysical Journal Supplement Series. 88: 383. Bibcode:1993ApJS...88..383L. doi:10.1086/191826. ISSN 0067-0049.
- ^ Kniazev, A Y; Egorova, E S; Pustilnik, S A (2018-07-02). "Study of galaxies in the Eridanus void. Sample and oxygen abundances". Monthly Notices of the Royal Astronomical Society. 479 (3): 3842–3857. arXiv:1809.05866. doi:10.1093/mnras/sty1704. ISSN 0035-8711.