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NGC 4869

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Elliptical galaxy in the constellation Coma Berenices
NGC 4869
The elliptical galaxy NGC 4869.
Observation data (J2000 epoch)
ConstellationComa Berenices
Right ascension12 59 23.36
Declination27° 54′ 41.78″
Redshift0.022820
Heliocentric radial velocity6,841 km/s
Distance343 Mly (105.16 Mpc)
Group or clusterComa Cluster
Apparent magnitude (V)13.52
Apparent magnitude (B)14.9
Characteristics
TypeE3, PAS
Size37.62 kiloparsecs (122,700 light-years)
(diameter; 2MASS K-band total isophote)
Notable featuresRadio 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: 105

NGC 4869 is an elliptical galaxy located in the constellation of Coma Berenices. It is located 343 million light years from Earth. 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. It is a member of the Coma Cluster with a small companion galaxy at a position angle of 325°.

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. It has an estimated γ-ray luminosity of Lγ ≤ 4 x 10 erg s like NGC 4874. There is also an elongated absorption feature in the galaxy, possibly representing an edge on disk.

NGC 4869 contains a narrow angle tailed radio source. The source is found lying towards the central region of the Coma Cluster by 111 kpc. It shows a mean fractional polarization of 18% at 4.535 GHz and 21% at 8.465 GHz and a large-scale structure that is almost 200 kpc. A characteristic feature of the source, is a sharp bend towards a north direction at 3’5 from the host galaxy's position.

According to a Chandra X-ray image of NGC 4869, a straight collimated jet is seen flaring when traversing a surface brightness edge.

Supermassive black hole

The supermassive black hole in NGC 4869 is estimated to be 1.32 x 10 Mʘ (10 Mʘ) based on a study made by Jong-Hak Woo and Urry in 2002.

References

  1. ^ "By Name NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved 2024-10-13.
  2. "New General Catalog Objects: NGC 4850 - 4899". cseligman.com. Retrieved 2024-10-13.
  3. ^ 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. arXiv:astro-ph/0009056. Bibcode:2000A&A...362..871C.
  4. de Juan, L.; Colina, L.; Perez-Fournon, I. (1994). "Surface photometry of low-luminosity radio galaxies". Astronomical Journal Supplement Series. 91 (2): 507–551. Bibcode:1994ApJS...91..507D. doi:10.1086/191947.
  5. ^ Lal, Dharam V. (2020-09-11). "NGC 4869 in the Coma Cluster: Twist, Wrap, Overlap, and Bend". The Astronomical Journal. 160 (4): 161. arXiv:2009.07146. Bibcode:2020AJ....160..161L. doi:10.3847/1538-3881/abacd1. ISSN 0004-6256.
  6. 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. arXiv:2110.00309. doi:10.1093/mnras/stac2266. ISSN 0035-8711.
  7. ^ 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. arXiv:1002.0594. Bibcode:2010A&A...513A..30B. doi:10.1051/0004-6361/200913696. ISSN 0004-6361.
  8. 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. Bibcode:1990A&A...232..337F. ISSN 0004-6361.
  9. Woo, Jong-Hak; Urry, C. Megan (November 2002). "AGN Black Hole Masses and Bolometric Luminosities". The Astronomical Journal. 576. arXiv:astro-ph/0207249. Bibcode:2002ApJ...579..530W. doi:10.1086/342878.

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