Jump to content

NGC 1596

From Wikipedia, the free encyclopedia
NGC 1596
NGC 1596 (right) by Legacy Surveys dr10
Observation data (J2000 epoch)
ConstellationDorado
Right ascension04h 27m 38.1s[1]
Declination−55° 01′ 40″[1]
Redshift0.005037 ± 0.000027 [1]
Heliocentric radial velocity1,510 ± 8 km/s[1]
Distance53.2 ± 16.1 Mly (16.3 ± 5.0 Mpc)[1]
Group or clusterDorado Group
Apparent magnitude (V)11.1[2]
Characteristics
TypeSA0: [1]
Apparent size (V)3.7 × 1.0[1]
Notable featuresInteracting with NGC 1602
Other designations
ESO 157-31, AM 0426-550, PGC 15153

NGC 1596 is a lenticular galaxy in the constellation Dorado. The galaxy lies about 55 million light years away from Earth, which means, given its apparent dimensions, that NGC 1596 is approximately 55,000 light years across.[1] It was discovered by John Herschel on December 5, 1834.[3] It is a member of the Dorado Group.[4]

The galaxy has a high-surface disk and a boxy bulge.[5] The boxy bulge is indicative of the presence of a bar.[6] The galaxy has an extended spheroidal envelope, which is more extending towards the southwest side than the northeast.[7] The ionised gas kinematics show the presence of counter-rotating gas.[8] The gas apparently was accreted by nearby galaxy NGC 1602 and has highly asymmetric distribution.[9] The galaxy doesn't have HII regions, but there is extended and [N II] emission.[10]

NGC 1596 forms a pair with magellanic spiral galaxy NGC 1602, lying at a distance of 3.1 arcminutes.[5] Hydrogen gas, as imaged in the hydrogen line (HI), has been found in an area around both galaxies and has two tidal tails, one to the north north-west and the other one to the north north-east of NGC 1602. The interaction started less than one billion years ago.[9]

References

[edit]
  1. ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 1596. Retrieved 6 February 2025.
  2. ^ "Revised NGC Data for NGC 1596". spider.seds.org. Retrieved 30 March 2024.
  3. ^ Seligman, Courtney. "NGC 1596 (= PGC 14965)". Celestial Atlas. Retrieved 19 November 2018.
  4. ^ Maia, M. A. G.; da Costa, L. N.; Latham, David W. (April 1989). "A catalog of southern groups of galaxies". The Astrophysical Journal Supplement Series. 69: 809. Bibcode:1989ApJS...69..809M. doi:10.1086/191328.
  5. ^ a b Sandage, A., Bedke, J. (1994), The Carnegie Atlas of Galaxies. Volume I, Carnegie Institution of Washington
  6. ^ Chung, Aeree; Bureau, M. (June 2004). "Stellar Kinematics of Boxy Bulges: Large-Scale Bars and Inner Disks". The Astronomical Journal. 127 (6): 3192–3212. arXiv:astro-ph/0403232. Bibcode:2004AJ....127.3192C. doi:10.1086/420988. {{cite journal}}: |last2= has generic name (help)
  7. ^ Pohlen, M.; Balcells, M.; Lütticke, R.; Dettmar, R.-J. (August 2004). "Thick disks of lenticular galaxies: 3D-photometric thin/thick disk decomposition of eight edge-on S0 galaxies". Astronomy & Astrophysics. 422 (2): 465–475. arXiv:astro-ph/0404164. Bibcode:2004A&A...422..465P. doi:10.1051/0004-6361:20035932.
  8. ^ Bureau, M.; Chung, A. (11 February 2006). "Discovery of counter-rotating gas in the galaxies NGC 1596 and 3203 and the incidence of gas counter-rotation in S0 galaxies". Monthly Notices of the Royal Astronomical Society. 366 (1): 182–188. arXiv:astro-ph/0512143. Bibcode:2006MNRAS.366..182B. doi:10.1111/j.1365-2966.2005.09840.x. {{cite journal}}: |last1= has generic name (help)
  9. ^ a b Chung, Aeree; Koribalski, Bärbel; Bureau, Martin; Van Gorkom, J. H. (26 June 2006). "Origin of the counterrotating gas in NGC 1596: Origin of the counterrotating gas in NGC 1596". Monthly Notices of the Royal Astronomical Society. 370 (3): 1565–1572. arXiv:astro-ph/0605600. doi:10.1111/j.1365-2966.2006.10579.x. {{cite journal}}: |last3= has generic name (help)
  10. ^ Rampazzo, R.; Ciroi, S.; Mazzei, P.; Di Mille, F.; Congiu, E.; Cattapan, A.; Bianchi, L.; Iodice, E.; Marino, A.; Plana, H.; Postma, J.; Spavone, M. (November 2020). "Dorado and its member galaxies: H α imaging of the group backbone". Astronomy & Astrophysics. 643: A176. arXiv:2009.14731. Bibcode:2020A&A...643A.176R. doi:10.1051/0004-6361/202038996.
[edit]