II Hz 4
| II Hz 4 | |
|---|---|
SDSS image of II Hz 4 | |
| Observation data (J2000 epoch) | |
| Constellation | Lynx |
| Right ascension | 08h 58m 33.04s[1] |
| Declination | +37° 05′ 11.45″[1] |
| Redshift | 0.042876[1] |
| Heliocentric radial velocity | 12,854 ± 4 km/s[1] |
| Distance | 617.3 ± 43.2 Mly (189.28 ± 13.25 Mpc) |
| magnitude (J) | 12.57[1] |
| Characteristics | |
| Type | Ring galaxy[1] |
| Size | ~233,000 ly (71.3 kpc) (estimated)[1] |
| Other designations | |
| CGCG 180-023, 2MASX J08583307+3705112, PGC 25211, NSA 036200, MaNGA 01-165561, ASK 206604.0[1] | |
II Hz 4 (short for II Herzog 4) is a ring galaxy located in the constellation of Lynx. The redshift of this galaxy is (z) 0.042[1] and it was first discovered by astronomer named Emil Herzog in 1963. It was also subsequently designated as II Hz 4 by Halton Arp who described as an unusual object.[2]
Description
II Hz 4 is categorized as a classical double ring galaxy, depicted as having an off-center nucleus within its ring structure and a secondary faint ring feature.[3][4][2][5] The nucleus galaxy is connected by two spiral arms that are described to have a faint appearance, with one of them shown as extended to join the ring feature located south.[4]
A separate low-surface brightness ring-like feature is seen, with its size exactly similar to the ring. There is an apparent galaxy companion located with the faint northern ring with an extension terminating at the edge of the second ring feature.[2] The rings have an approximate size of 21.6 x 15.7 and 22.8 and 16.9 kiloparsecs when imaged in both K-band and hydrogen-alpha imaging.[4] A tidal tail with a blue appearance is seen connecting to the companion hinting an interaction.[3]
A study published in December 1998, has found the presence of ring knots in the galaxy. Based on observations, the estimated model ages of the knots are between six and eight million years.[6] Evidence also found, the two nuclei of the galaxy have a recession velocity differences of 50 kilometers per seconds, with the primary ring feature being inclined at 42° and has a rotation velocity of 28 kilometers per seconds.[7]
References
- ^ a b c d e f g h i "NED Search results for II Hz 4". NASA/IPAC Extragalactic Database. Retrieved 2026-03-19.
- ^ a b c Lynds, R.; Toomre, A. (October 1976). "On the interpretation of ring galaxies: the binary ring system II Hz 4". The Astrophysical Journal. 209: 382–388. doi:10.1086/154730. ISSN 0004-637X.
- ^ a b Appleton, P. N.; Marston, A. P. (January 1997). "Multiwavelength Observations of Collisional Ring Galaxies.I.Broad-Band Images, Global Properties, and Radial Colors of the Sample Galaxies". The Astronomical Journal. 113: 201–224. doi:10.1086/118245. ISSN 0004-6256.
- ^ a b c Marston, A. P.; Appleton, P. N. (March 1995). "Multiwavelength Observations of Ring Galaxies. II. Global Star Formation in Ring Galaxies". The Astronomical Journal. 109: 1002. doi:10.1086/117337. ISSN 0004-6256.
- ^ Romano, R.; Mayya, Y. D.; Vorobyov, E. I. (September 2008). "Stellar Disks of Collisional Ring Galaxies. I. New Multiband Images, Radial Intensity and Color Profiles, and Confrontation with N-Body Simulations". The Astronomical Journal. 136 (3): 1259–1289. doi:10.1088/0004-6256/136/3/1259. ISSN 0004-6256.
- ^ Bransford, M. A.; Appleton, P. N.; Marston, A. P.; Charmandaris, V. (December 1998). "Multiwavelength Observations of Collisional Ring Galaxies. III. Oxygen/Nitrogen Abundances and Star Formation Properties of Ring Knots". The Astronomical Journal. 116 (6): 2757–2775. doi:10.1086/300629. ISSN 0004-6256.
- ^ Horellou, C.; Casoli, F.; Combes, F.; Dupraz, C. (June 1995). "The CO emission of ring galaxies". Astronomy and Astrophysics. 298: 743. ISSN 0004-6361.
External links
- II Hz 4 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images