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NGC 1574

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NGC 1574
NGC 1574 by the Legacy Survey DR10
Observation data (J2000 epoch)
ConstellationReticulum
Right ascension04h 21m 58.7s[1]
Declination−56° 58′ 28″[1]
Redshift0.003472 ± 0.000053 [1]
Heliocentric radial velocity1,041 ± 16 km/s[1]
Distance53.7 ± 19.1 Mly (16.5 ± 5.9 Mpc)[1]
Group or clusterDorado Group
Apparent magnitude (V)10.3[2]
Characteristics
TypeSA0^- [1]
Apparent size (V)3.4 × 3.1[1]
Other designations
ESO 157-22, AM 0421-570, IRAS F04210-5705, PGC 14965

NGC 1574 is a lenticular galaxy in the constellation Reticulum. The galaxy lies about 55 million light years away from Earth, which means, given its apparent dimensions, that NGC 1574 is approximately 75,000 light years across.[1] It was discovered by John Herschel on December 4, 1834.[3] It is a member of the Dorado Group.[4]

The galaxy features a bar embedded in an extended disk. A nearly complete ring surrounds the bar.[5] The galaxy is seen nearly face-on, at an inclination of about 27°. Carbon monoxide gas has been lying in a disk about 2.6 arcseconds across, which corresponds to about 200 parsecs, around the nucleus. The kinematics suggest that it is due to a warp in the disk. The nucleus of the galaxy doesn't appear to be active. The supermassive black hole is estimated to have a mass of (1.0±0.2)×108 M.[6]

References

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  1. ^ a b c d e f g h "NASA/IPAC Extragalactic Database". Results for NGC 1574. Retrieved 6 February 2025.
  2. ^ "Revised NGC Data for NGC 1574". spider.seds.org. Retrieved 30 March 2024.
  3. ^ Seligman, Courtney. "NGC 1574 (= 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. ^ Laurikainen, Eija; Salo, Heikki; Buta, Ronald; Knapen, Johan; Speltincx, Tom; Block, David (January 2006). "Morphology of 15 Southern Early?Type Disk Galaxies". The Astronomical Journal. 132 (6): 2634–2652. arXiv:astro-ph/0609343. Bibcode:2006AJ....132.2634L. doi:10.1086/508810.
  6. ^ Ruffa, Ilaria; Davis, Timothy A; Cappellari, Michele; Bureau, Martin; Elford, Jacob; Iguchi, Satoru; Lelli, Federico; Liang, Fu-Heng; Liu, Lijie; Lu, Anan; Sarzi, Marc; Williams, Thomas G (11 May 2023). "WISDOM project – XIV. SMBH mass in the early-type galaxies NGC 0612, NGC 1574, and NGC 4261 from CO dynamical modelling". Monthly Notices of the Royal Astronomical Society. 522 (4): 6170–6195. doi:10.1093/mnras/stad1119. {{cite journal}}: |last4= has generic name (help)
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