Astronomy:NGC 4698

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Short description: Galaxy in the constellation Virgo
NGC 4698
N4698s.jpg
NGC 4698 imaged with the 32-inch Schulman Telescope at Mount Lemmon Observatory
Observation data (J2000 epoch)
ConstellationVirgo
Right ascension 12h 34m 20.310s[1]
Declination+08° 11′ 51.94″[1]
Helio radial velocity1,002[2] km/s
Distance54.8 Mly (16.8 Mpc)[3]
Group or clusterVirgo Cluster
Apparent magnitude (V)10.6[4]
Apparent magnitude (B)11.46[5]
Characteristics
TypeSA(s)ab[3]
Apparent size (V)4′.0 × 2′.9[4]
Notable featuresSeyfert-2 galaxy[6]
Other designations
PGC 43254, UGC 7970, VCC 2070

NGC 4698 is a barred spiral galaxy[5] located around 55[3] million light years away from Earth in the constellation of Virgo. It belongs to the Virgo Cluster of galaxies and is positioned near the northeastern edge of this assemblage.[4] The morphological classification of NGC 4698 in the De Vaucouleurs system is SA(s)ab,[3] which indicates a purely spiral structure with moderate to tightly wound arms.[7] It is inclined to the line of sight from the Earth by an angle of 53° along a position angle of 170°.[8]

A unique feature of this galaxy is that the stars and dust of the nuclear disk are rotating in a direction that is aligned perpendicularly to the galactic disk. The bulge likewise appears elongated out of the galactic plane. This unusual alignment may have been the result of a past merger event.[5]

NGC 4698 is classified as a Seyfert-2 galaxy with an active galactic nucleus, which displays a prominent emission of radio and X-ray energy from the core while showing narrow emission lines in the optical spectrum.[6] The unified model of Seyfert galaxies proposes that the nucleus of a Seyfert 2 galaxy is obscured by a thick torus of gas and dust. However, the varying X-ray emission of the core of NGC 4698 shows little indication of being obstructed, suggesting instead that the source of the energy emission is generally unobscured but anemic in nature.[9]

Gallery

References

  1. 1.0 1.1 Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W. et al. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal 131 (2): 1163–1183. doi:10.1086/498708. ISSN 0004-6256. Bibcode2006AJ....131.1163S. https://ui.adsabs.harvard.edu/abs/2006AJ....131.1163S/abstract. 
  2. Crook, Aidan C. et al. (February 2007), "Groups of Galaxies in the Two Micron All Sky Redshift Survey", The Astrophysical Journal 655 (2): 790–813, doi:10.1086/510201, Bibcode2007ApJ...655..790C. 
  3. 3.0 3.1 3.2 3.3 de Looze, Ilse et al. (October 2011), "The reliability of [C II] as an indicator of the star formation rate", Monthly Notices of the Royal Astronomical Society 416 (4): 2712–2724, doi:10.1111/j.1365-2966.2011.19223.x, Bibcode2011MNRAS.416.2712D. 
  4. 4.0 4.1 4.2 Finlay, W. H. (2003), Concise Catalog of Deep-sky Objects: Astrophysical Information for 500 Galaxies, Clusters and Nebulae, Springer, p. 175, ISBN 978-1852336912, https://books.google.com/books?id=t35J1QRSFAEC&pg=PT180. 
  5. 5.0 5.1 5.2 Corsini, E. M. et al. (June 2012), "Polar bulges and polar nuclear discs: the case of NGC 4698", Monthly Notices of the Royal Astronomical Society: Letters 423 (1): L79–L83, doi:10.1111/j.1745-3933.2012.01261.x, Bibcode2012MNRAS.423L..79C. 
  6. 6.0 6.1 Georgantopoulos, I. et al. (September 2003), "Chandra Observations of NGC 4698: A Seyfert 2 Galaxy with No Absorption", The Astrophysical Journal 594 (2): 704–708, doi:10.1086/377120, Bibcode2003ApJ...594..704G. 
  7. Buta, Ronald J. et al. (2007), Atlas of Galaxies, Cambridge University Press, pp. 13–17, ISBN 978-0521820486, https://books.google.com/books?id=g-P7dCbB5MEC&pg=PA16. 
  8. Giovanardi, C. et al. (March 1996), "Near-Infrared Low-Resolution Mapping of Early-Type Spirals", Astronomical Journal 111 (2): 1086–1097, doi:10.1086/117854, Bibcode1996AJ....111.1086G. 
  9. Tran, Hien D. et al. (January 2011), "Indecent Exposure in Seyfert 2 Galaxies: A Close Look", The Astrophysical Journal Letters 726 (2): L21, doi:10.1088/2041-8205/726/2/L21, Bibcode2011ApJ...726L..21T. 

External links