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NGC 1433

NGC 1433 (also known as PGC 13586) is a barred spiral galaxy with a double ring structure located in the constellation of Horologium. It is at a distance of 46 million light-years from Earth.[4] It 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.[5] NGC 1433 is being studied as part of a survey of 50 nearby galaxies known as the Legacy ExtraGalactic UV Survey (LEGUS).[6] 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.[7]

NGC 1433
Composite view of the galaxy NGC 1433 from ALMA and the Hubble Space Telescope[1]
Observation data (J2000 epoch)
ConstellationHorologium
Right ascension03h 42m 01.553s[2]
Declination−47° 13′ 19.49″[2]
Redshift0.003590[2]
Heliocentric radial velocity1076±1 km/s[3]
Distance46.2 ± 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 was discovered by James Dunlop in 1826. One supernova has been observed in NGC 1433, SN 1985 P, type II with apparent magnitude 13.5 at discovery, on 10 October 1985.[8]

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

Gallery edit

References edit

  1. ^ "ALMA Probes Mysteries of Jets from Giant Black Holes". ESO Press Release. Retrieved 18 October 2013.
  2. ^ a b c d e "Search Results for NGC 1433". Astronomical Database. SIMBAD. Retrieved 18 October 2013.
  3. ^ a b c "NASA/IPAC Extragalactic Database". Results for NGC 1433. Retrieved 2016-01-18.
  4. ^ a b c 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. ^ 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.
  6. ^ "Legacy ExtraGalactic UV Survey (LEGUS site)". website. Retrieved 21 Oct 2016.
  7. ^ a b "A galaxy with a glowing heart". ESA/Hubble Picture of the Week. Retrieved 8 August 2014.
  8. ^ Spectroscopy and photometry of a type II supernova 1985P in NGC1433 Workshop of ESO for SN 1987A, Garching, Federal Republic of Germany, 6-8 Ιουλίου 1987, Proceedings (A88-35301 14-90). Garching, Federal Republic of Germany, European Southern Observatory, 1987, p. 655-661.
  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.

External links edit

  •   Media related to NGC 1433 at Wikimedia Commons


1433, also, known, 13586, barred, spiral, galaxy, with, double, ring, structure, located, constellation, horologium, distance, million, light, years, from, earth, seyfert, galaxy, with, active, galactic, nucleus, central, region, galaxy, displays, intense, sta. NGC 1433 also known as PGC 13586 is a barred spiral galaxy with a double ring structure located in the constellation of Horologium It is at a distance of 46 million light years from Earth 4 It 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 5 NGC 1433 is being studied as part of a survey of 50 nearby galaxies known as the Legacy ExtraGalactic UV Survey LEGUS 6 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 7 NGC 1433Composite view of the galaxy NGC 1433 from ALMA and the Hubble Space Telescope 1 Observation data J2000 epoch ConstellationHorologiumRight ascension03h 42m 01 553s 2 Declination 47 13 19 49 2 Redshift0 003590 2 Heliocentric radial velocity1076 1 km s 3 Distance46 2 3 8 Mly 14 15 1 15 Mpc 4 Apparent magnitude V 9 99 2 Apparent magnitude B 10 84 2 CharacteristicsType R 1 SB rs ab 3 Apparent size V 6 5 5 9 3 Other designationsHIPASS 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 was discovered by James Dunlop in 1826 One supernova has been observed in NGC 1433 SN 1985 P type II with apparent magnitude 13 5 at discovery on 10 October 1985 8 NGC 1433 is member of the Dorado Group 4 9 Gallery edit nbsp LEGUS optical 7 nbsp Hubble Space Telescope optical nbsp STSci DSS optical nbsp James Webb Space Telescope MIRI compass References edit ALMA Probes Mysteries of Jets from Giant Black Holes ESO Press Release Retrieved 18 October 2013 a b c d e Search Results for NGC 1433 Astronomical Database SIMBAD Retrieved 18 October 2013 a b c NASA IPAC Extragalactic Database Results for NGC 1433 Retrieved 2016 01 18 a b c 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 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 amp A 391 83B doi 10 1051 0004 6361 20020642 S2CID 14749261 Legacy ExtraGalactic UV Survey LEGUS site website Retrieved 21 Oct 2016 a b A galaxy with a glowing heart ESA Hubble Picture of the Week Retrieved 8 August 2014 Spectroscopy and photometry of a type II supernova 1985P in NGC1433 Workshop of ESO for SN 1987A Garching Federal Republic of Germany 6 8 Ioylioy 1987 Proceedings A88 35301 14 90 Garching Federal Republic of Germany European Southern Observatory 1987 p 655 661 ALMA observations of feeding and feedback in nearby Seyfert galaxies an AGN driven outflow in NGC 1433 PDF Manuscript no nugas1 Astronomy amp Astronophysics Retrieved 18 October 2013 External links edit nbsp Media related to NGC 1433 at Wikimedia Commons nbsp This spiral galaxy article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title NGC 1433 amp oldid 1192866569, wikipedia, wiki, book, books, library,

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