Astronomy:NGC 2326
| NGC 2326 | |
|---|---|
 NGC 2326 (top right) and NGC 2326A (UGC 3687) with legacy surveys | |
| Observation data (J2000 epoch) | |
| Constellation | Lynx |
| Right ascension | 07h 08m 11.0037s[1] |
| Declination | +50° 40′ 54.994″[1] |
| Redshift | 0.019960[1] |
| Helio radial velocity | 5924 km/s[2] |
| Distance | 291.6 ± 20.4 Mly (89.41 ± 6.26 Mpc)[1] |
| Apparent magnitude (V) | 13.2[1] |
| Apparent magnitude (B) | 14.3[2] |
| Characteristics | |
| Type | SB(rs)b[1] |
| Size | ~267,500 ly (82.01 kpc) (estimated)[1] |
| Apparent size (V) | 1.9′ × 1.8′[1] |
| Other designations | |
| IRAS F07043+5045, UGC 3681, MCG+08-13-062, PGC 20218[1] | |
Coordinates: 
07h 08m 11.0037s, +50° 40′ 54.994″
NGC 2326 is a barred spiral galaxy in the Lynx constellation. Its velocity with respect to the cosmic microwave background is 6062 ± 11 km/s, which corresponds to a Hubble distance of 291.6 ± 20.4 Mly (89.41 ± 6.26 Mpc).[1] It was discovered by William Herschel on 9 February 1788.[3] Its apparent magnitude is 14.3 [2] and its size is 2.71 arc minutes.[2] It is located near NGC 2326A.
The SIMBAD database lists NGC 2326 as a radio galaxy, i.e. it has giant regions of radio emission extending well beyond its visible structure.[4]
HDC 426 Group
NGC 2326 is a member of a group of galaxies known as [CHM2007] HDC 426. This group contains 18 galaxies, including NGC 2315, NGC 2320, NGC 2321 (fr), NGC 2322 (fr), NGC 2332 (fr), NGC 2340, IC 458 (de), and IC 465 (de).[5][6] NGC 2326 is also a member of the galaxy cluster Abell 569.[7][8]
Supernova
One supernova has been observed in NGC 2326. SN 2023pgb (Type II, mag. 17.44) was discovered by the Zwicky Transient Facility on 12 August 2023.[9]
See also
References
- ↑ 1.00 1.01 1.02 1.03 1.04 1.05 1.06 1.07 1.08 1.09 "Results for object NGC 2326". NASA and Caltech. http://ned.ipac.caltech.edu/byname?objname=NGC+2326.
- ↑ 2.0 2.1 2.2 2.3 "NGC 2326 -- Radio Galaxy". SIMBAD. http://simbad.u-strasbg.fr/simbad/sim-id?Ident=NGC++2326.
- ↑ "NGC 2326 (= PGC 20218)". cseligman. http://cseligman.com/text/atlas/ngc23.htm#2326.
- ↑ "NGC 2326". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=NGC+2326.
- ↑ Crook, Aidan C.; Huchra, John P.; Martimbeau, Nathalie; Masters, Karen L.; Jarrett, Tom; Macri, Lucas M. (2007). "Groups of Galaxies in the Two Micron All Sky Redshift Survey". The Astrophysical Journal 655 (2): 790–813. doi:10.1086/510201. Bibcode: 2007ApJ...655..790C.
- ↑ "[CHM2007 HDC 426"]. SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=%5BCHM2007%5D+HDC+426.
- ↑ Sakai, Shoko; Kennicutt, Robert C., Jr.; Moss, Chris (2012). "A Deep, Wide-field Hα Survey of Nearby Clusters of Galaxies: Data". The Astrophysical Journal Supplement Series 199 (2): 36. doi:10.1088/0067-0049/199/2/36. Bibcode: 2012ApJS..199...36S.
- ↑ "ACO 569". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=ACO+569.
- ↑ "SN 2023pgb". IAU. https://www.wis-tns.org/object/2023pgb.
Template:NGC objects:2001-3000
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