Astronomy:NGC 4869
| NGC 4869 | |
|---|---|
 The elliptical galaxy NGC 4869. | |
| Observation data (J2000 epoch) | |
| Constellation | Coma Berenices |
| Right ascension | 12h 59m 23.36s |
| Declination | 27° 54′ 41.78″ |
| Redshift | 0.022820 |
| Helio radial velocity | 6,841 km/s |
| Distance | 343 Mly (105.16 Mpc) |
| Group or cluster | Coma Cluster |
| Apparent magnitude (V) | 13.52 |
| Apparent magnitude (B) | 14.9 |
| Characteristics | |
| Type | E3, PAS |
| Size | 37.62 kiloparsecs (122,700 light-years) (diameter; 2MASS K-band total isophote)[1] |
| Notable features | Radio galaxy |
| Other designations | |
| MCG +05-31-065, CGCG 160-225, PGC 44587, B2 1256+58, 5C 04.081, TXS 1257+281, 7C 1256+2810, KUG 1256+375, ABELL 1656:[D80] 105 | |
NGC 4869 is an elliptical galaxy located in the constellation of Coma Berenices. It is located 343 million light years from Earth.[1] The galaxy was discovered by William Herschel in April 1785 but also observed by both John Herschel and Heinrich d'Arrest, in March 1827 and May 1863 respectively.[2] It is a member of the Coma Cluster[1][3] with a small companion galaxy at a position angle of 325°.[4]
Characteristics
NGC 4869 is classified as a radio galaxy with a faint radio core with two oppositely directed radio jets and a lengthy low-surface brightness tail.[5] It has an estimated γ-ray luminosity of Lγ ≤ 4 x 1039 erg s−1 like NGC 4874.[6] There is also an elongated absorption feature in the galaxy, possibly representing an edge on disk.[3]
NGC 4869 contains a narrow angle tailed radio source.[7][8] The source is found lying towards the central region of the Coma Cluster by 111 kpc.[5] It shows a mean fractional polarization of 18% at 4.535 GHz and 21% at 8.465 GHz[7] and a large-scale structure that is almost 200 kpc.[5] A characteristic feature of the source, is a sharp bend towards a north direction at 3’5 from the host galaxy's position.[5]
According to a Chandra X-ray image of NGC 4869, a straight collimated jet is seen flaring when traversing a surface brightness edge.[5]
Supermassive black hole
The supermassive black hole in NGC 4869 is estimated to be 1.32 x 108 Mʘ (108.12 Mʘ) based on a study made by Jong-Hak Woo and Urry in 2002.[9]
References
- ↑ 1.0 1.1 1.2 "By Name NASA/IPAC Extragalactic Database". http://ned.ipac.caltech.edu/byname?objname=NGC+4869&hconst=67.8&omegam=0.308&omegav=0.692&wmap=4&corr_z=1.
- ↑ "New General Catalog Objects: NGC 4850 - 4899". https://cseligman.com/text/atlas/ngc48a.htm#4869.
- ↑ 3.0 3.1 Capetti, A.; de Ruiter, H.R.; Fanti, R.; Morganti, R.; Parma, P.; Ulrich, M.-H. (2000). "The HST snapshot survey of the B2 sample of low luminosity radio-galaxies: a picture gallery". Astronomy & Astrophysics 362: 871–885. Bibcode: 2000A&A...362..871C. https://articles.adsabs.harvard.edu//full/2000A%26A...362..871C/0000882.000.html.
- ↑ de Juan, L.; Colina, L.; Perez-Fournon, I. (1994). "Surface photometry of low-luminosity radio galaxies". The Astrophysical Journal Supplement Series 91 (2): 507–551. doi:10.1086/191947. Bibcode: 1994ApJS...91..507D. https://articles.adsabs.harvard.edu//full/1994ApJS...91..507D/0000547.000.html.
- ↑ 5.0 5.1 5.2 5.3 5.4 Lal, Dharam V. (2020-09-11). "NGC 4869 in the Coma Cluster: Twist, Wrap, Overlap, and Bend". The Astronomical Journal 160 (4): 161. doi:10.3847/1538-3881/abacd1. ISSN 0004-6256. Bibcode: 2020AJ....160..161L.
- ↑ Baghmanyan, Vardan; Zargaryan, Davit; Aharonian, Felix; Yang, Ruizhi; Casanova, Sabrina; Mackey, Jonathan (2022-08-13). "Detailed study of extended γ-ray morphology in the vicinity of the Coma cluster with Fermi Large Area Telescope". Monthly Notices of the Royal Astronomical Society 516 (1): 562–571. doi:10.1093/mnras/stac2266. ISSN 0035-8711.
- ↑ 7.0 7.1 Bonafede, A.; Feretti, L.; Murgia, M.; Govoni, F.; Giovannini, G.; Dallacasa, D.; Dolag, K.; Taylor, G. B. (April 2010). "The Coma cluster magnetic field from Faraday rotation measures". Astronomy and Astrophysics 513: A30. doi:10.1051/0004-6361/200913696. ISSN 0004-6361. Bibcode: 2010A&A...513A..30B. http://dx.doi.org/10.1051/0004-6361/200913696.
- ↑ Feretti, L.; Dallacasa, D.; Giovannini, G.; Venturi, T. (June 1990). "Astrophysical implications of the study of the tailed radio source NGC 4869 in the Coma cluster". Astronomy & Astrophysics 232 (2): 337–343. ISSN 0004-6361. Bibcode: 1990A&A...232..337F. https://articles.adsabs.harvard.edu/full/1990A%26A...232..337F.
- ↑ Woo, Jong-Hak; Urry, C. Megan (November 2002). "AGN Black Hole Masses and Bolometric Luminosities". The Astrophysical Journal 576 (2): 530. doi:10.1086/342878. Bibcode: 2002ApJ...579..530W.
External links
- NGC 4869 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- NGC 4869 on SIMBAD
Template:NGC objects:4500-4999
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