NGC 1433

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NGC 1433
Composite view of the galaxy NGC 1433 from ALMA and Hubble.jpg
Composite view of the galaxy NGC 1433 from ALMA and the Hubble Space Telescope [1]
Observation data (J2000 epoch)
Constellation Horologium
Right ascension 03h 42m 01.553s [2]
Declination −47° 13′ 19.49″ [2]
Redshift 0.003590 [2]
Heliocentric radial velocity 1076±1 km/s [3]
Distance 46.2 ± 3.8  Mly (14.15 ± 1.15  Mpc) [4]
Apparent magnitude  (V)9.99 [2]
Apparent magnitude  (B)10.84 [2]
Characteristics
Type (R'_1)SB(rs)ab [3]
Apparent size  (V)6.5′ × 5.9′ [3]
Other designations
HIPASS J0342-47, QDOT B0340269-472245, [CHM2007] LDC 266, J034201.55-4713194, AM 0340-472, IRAS 03404-4722, SGC 034027-4722.8, [VDD93] 31, 6dFGS gJ034201.5-471319, LEDA 13586, SINGG HIPASS J0342-47, ESO 249-14, 2MASX J03420155-4713194, [A81] 034029-4724, ESO-LV 249-0140, PSCz Q03404-4722, [CHM2007] HDC 257 J034201.55-4713194

NGC 1433 (also known as PGC 13586) is a barred spiral galaxy with a double ring structure located in the constellation of Horologium. It was discovered by James Dunlop on 28 September 1826, [5] and lies a distance of 46 million light-years from Earth. [4]

Contents

NGC 1433 is a Seyfert galaxy with an active galactic nucleus. The central region of the galaxy displays intense star formation activity, with an irregular star-forming ring of 5″ (or 0.3 kpc) radius and weak radio wave emission. Star formation is also noticeable in the spiral arms but not the bar of the galaxy. [6] NGC 1433 is being studied as part of a survey of 50 nearby galaxies known as the Legacy ExtraGalactic UV Survey (LEGUS). [7] A jet of material flowing away from the central black hole of the galaxy extending for only 150 light-years has been found. It is the smallest molecular outflow ever observed in a galaxy beyond our own. [8]

NGC 1433 is member of the Dorado Group. [4] [9]

Supernova

One supernova has been observed in NGC 1433. SN 1985P (Type II, mag. 13.5) was discovered by Robert Evans on 10 October 1985. [10] [11] [12]

References

  1. ↑ "ALMA Probes Mysteries of Jets from Giant Black Holes". ESO Press Release. Retrieved 18 October 2013.
  2. 1 2 3 4 5 "Search Results for NGC 1433". Astronomical Database. SIMBAD . Retrieved 18 October 2013.
  3. 1 2 3 "NASA/IPAC Extragalactic Database". Results for NGC 1433. Retrieved 2016-01-18.
  4. 1 2 3 Tikhonov, N. A.; Galazutdinova, O. A. (2020). "Distance to the Dorado Group". Astrophysical Bulletin. 75 (4): 384–393. arXiv: 2009.04090 . Bibcode:2020AstBu..75..384T. doi:10.1134/S199034132004015X. S2CID   221556782.
  5. ↑ Seligman, Courtney. "New General Catalogue Objects: NGC 1433". Celestial Atlas. Retrieved 25 November 2024.
  6. ↑ Beck, R.; Shoutenkov, V.; Ehle, M.; Harnett, J. I.; Haynes, R. F.; Shukurov, A.; et al. (August 2002). "Magnetic fields in barred galaxies. I. The atlas" (PDF). Astronomy and Astrophysics. 391: 83–102. arXiv: astro-ph/0207201 . Bibcode:2002A&A...391...83B. doi:10.1051/0004-6361:20020642. S2CID   14749261.
  7. ↑ "Legacy ExtraGalactic UV Survey (LEGUS site)". website. Retrieved 21 Oct 2016.
  8. 1 2 "A galaxy with a glowing heart". ESA/Hubble Picture of the Week. Retrieved 8 August 2014.
  9. ↑ "ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow in NGC 1433" (PDF). Manuscript no. nugas1. Astronomy & Astronophysics. Retrieved 18 October 2013.
  10. ↑ Evans, R. O.; Thompson, G. (1985). "Supernova 1985P in NGC 1433". International Astronomical Union Circular (4119): 2. Bibcode:1985IAUC.4119....2E.
  11. ↑ Chalabaev, A. A.; Cristiani, S. (1987). "Spectroscopy and Photometry of a Type-II Supernova 1985P in NGC1433". European Southern Observatory Conference and Workshop Proceedings. 26: 655. Bibcode:1987ESOC...26..655C.
  12. ↑ "SN 1985P". Transient Name Server. IAU . Retrieved 5 December 2024.


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