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Coordinates: Sky map 03h 42m 01.553s, −47° 13′ 19.49″
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{{Short description|Barred spiral galaxy in the constellation Horologium}}
{{Short description|Galaxy in the constellation Horologium}}
{{Sky|03|42|01.553|-|47|13|19.49}}
{{Sky|03|42|01.553|-|47|13|19.49}}

{{Infobox galaxy
{{Infobox galaxy
| name = NGC 1433 (PGC 13586 - Miltron's Galaxy)
| name = NGC 1433
| image = Composite view of the galaxy NGC 1433 from ALMA and Hubble.jpg
| image = Composite view of the galaxy NGC 1433 from ALMA and Hubble.jpg
⚫
| caption = Composite view of the galaxy NGC 1433 from [[Atacama Large Millimeter Array|ALMA]] and the [[Hubble Space Telescope]]<ref>{{cite news|title=ALMA Probes Mysteries of Jets from Giant Black Holes|url=http://www.eso.org/public/news/eso1344/|access-date=18 October 2013|newspaper=ESO Press Release}}</ref>
| image_size = 300px
⚫
| caption = Composite view of the galaxy NGC 1433 from [[Atacama Large Millimeter Array|ALMA]] and [[Hubble Space Telescope|Hubble]]<ref>{{cite news|title=ALMA Probes Mysteries of Jets from Giant Black Holes|url=http://www.eso.org/public/news/eso1344/|access-date=18 October 2013|newspaper=ESO Press Release}}</ref>
| credit = ALMA (ESO/NAOJ/NRAO)/NASA/ESA/F. Combes
| epoch = [[J2000]]
| epoch = [[J2000]]
| pronounce =
| pronounce =
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| h_radial_v = 1076±1 km/s<ref name="ned" />
| h_radial_v = 1076±1 km/s<ref name="ned" />
| gal_v =
| gal_v =
| dist_ly = {{cvt|14.15|±|1.15|Mpc|Mly|lk=on|order=flip}}<ref name=Tikhonov>{{cite journal|doi=10.1134/S199034132004015X|title=Distance to the Dorado Group|year=2020|last1=Tikhonov|first1=N. A.|last2=Galazutdinova|first2=O. A.|journal=Astrophysical Bulletin|volume=75|issue=4|pages=384–393|arxiv=2009.04090|bibcode=2020AstBu..75..384T|s2cid=221556782}}</ref>
⚫
| dist_ly = 32 Mly<ref name=hst>{{cite web|title=A galaxy with a glowing heart (HST site)|url=http://www.spacetelescope.org/images/potw1427a/|work=website|access-date=17 July 2014}}</ref>
| group_cluster =
| group_cluster =
| type = (R'_1)SB(rs)ab <ref name="ned">{{cite web
| type = (R'_1)SB(rs)ab <ref name="ned">{{cite web
Line 29: Line 26:
| appmag_b = 10.84<ref name=simbad/>
| appmag_b = 10.84<ref name=simbad/>
| absmag_v =
| absmag_v =
| size_v = 6′.5 × 5′.9<ref name="ned" />
| size_v = 6.5{{prime}} × 5.9{{prime}}<ref name="ned" />
| notes =
| notes =
| names = HIPASS J0342-47, QDOT B0340269-472245, [CHM2007] LDC 266, J034201.55-4713194,
| names = 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
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
| references =
| references =
}}
}}
'''NGC 1433''' (also known as PGC 13586) is a [[barred spiral galaxy]] with a double ring structure located in the constellation of [[Horologium (constellation)|Horologium]]. It was discovered by [[James Dunlop]] on 28 September 1826,<ref name="selig">{{cite web | url = https://cseligman.com/text/atlas/ngc14.htm#1433 | title = New General Catalogue Objects: NGC{{nbsp}}1433 | last = Seligman | first = Courtney | website = Celestial Atlas | access-date = 25 November 2024}}</ref> and lies a distance of 46 million [[light-year]]s from Earth.<ref name=Tikhonov/>


'''NGC 1433''' (also known as '''PGC 13586''' or '''Miltron's Galaxy''') is a [[barred spiral galaxy]] with a double ring structure located in the constellation of [[Horologium (constellation)|Horologium]]. It is at a distance of 30 million [[light years]] from Earth. It is a [[Seyfert galaxy]] with an active galactic nuclei. The central region of the galaxy portraits 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.<ref>{{cite journal | url=http://www.aanda.org/articles/aa/pdf/2002/31/aa2373.pdf | title=Magnetic fields in barred galaxies. I. The atlas | display-authors=6 | author=Beck, R. | author2=Shoutenkov, V. | author3=Ehle, M. | author4=Harnett, J. I. | author5=Haynes, R. F. | author6=Shukurov, A. | author7=Sokoloff, D. D. | author8=Thierbach, M. | journal=Astronomy and Astrophysics | date = August 2002 | volume=391 | pages=83–102 | doi=10.1051/0004-6361:20020642|arxiv = astro-ph/0207201 |bibcode = 2002A&A...391...83B }}</ref> NGC 1433 is being studied as part of a survey of 50 nearby galaxies known as the Legacy ExtraGalactic UV Survey (LEGUS).<ref name=LEGUS>{{cite web|title=Legacy ExtraGalactic UV Survey (LEGUS site)|url=https://legus.stsci.edu//|work=website|access-date=21 Oct 2016}}</ref> 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.<ref name=POTW1427a/>
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{{pprime}} (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.<ref>{{cite journal | url=http://www.aanda.org/articles/aa/pdf/2002/31/aa2373.pdf | title=Magnetic fields in barred galaxies. I. The atlas | display-authors=6 | author=Beck, R. | author2=Shoutenkov, V. | author3=Ehle, M. | author4=Harnett, J. I. | author5=Haynes, R. F. | author6=Shukurov, A. | author7=Sokoloff, D. D. | author8=Thierbach, M. | journal=Astronomy and Astrophysics | date = August 2002 | volume=391 | pages=83–102 | doi=10.1051/0004-6361:20020642|arxiv = astro-ph/0207201 |bibcode = 2002A&A...391...83B | s2cid=14749261 }}</ref> NGC 1433 is being studied as part of a survey of 50 nearby galaxies known as the Legacy ExtraGalactic UV Survey (LEGUS).<ref name=LEGUS>{{cite web|title=Legacy ExtraGalactic UV Survey (LEGUS site)|url=https://legus.stsci.edu//|work=website|access-date=21 Oct 2016}}</ref> 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.<ref name=POTW1427a/>


One [[supernova]] has been observed in NGC 1433. SN{{nbsp}}1985P ([[Type_II_supernova|type{{nbsp}}II]], mag. 13.5) was discovered by [[Robert_Evans_(astronomer)|Robert Evans]] on 10 October 1985.<ref>{{cite journal | bibcode=1985IAUC.4119....2E| title=Supernova 1985P in NGC 1433| last1=Evans| first1=R. O.| last2=Thompson| first2=G.| journal=International Astronomical Union Circular| date=1985| issue=4119| page=2}}</ref><ref>{{cite journal | bibcode=1987ESOC...26..655C| title=Spectroscopy and Photometry of a Type-II Supernova 1985P in NGC1433| last1=Chalabaev| first1=A. A.| last2=Cristiani| first2=S.| journal=European Southern Observatory Conference and Workshop Proceedings| date=1987| volume=26| page=655}}</ref><ref>{{cite web | website=Transient Name Server | title=SN{{nbsp}}1985P | url=https://www.wis-tns.org/object/1985P | publisher = [[International_Astronomical_Union|IAU]] | access-date=5 December 2024}}</ref>
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.<ref>[http://adsabs.harvard.edu/abs/1987ESOC...26..655C 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.</ref>


NGC 1433 is member of the [[Dorado Group]].<ref>{{cite web|title=ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow in NGC 1433|url=http://www.eso.org/public/archives/releases/sciencepapers/eso1344/eso1344a.pdf|work=Manuscript no. nugas1|publisher=Astronomy & Astronophysics|access-date=18 October 2013}}</ref>
NGC 1433 is member of the [[Dorado Group]].<ref name=Tikhonov/><ref>{{cite web|title=ALMA observations of feeding and feedback in nearby Seyfert galaxies: an AGN-driven outflow in NGC 1433|url=http://www.eso.org/public/archives/releases/sciencepapers/eso1344/eso1344a.pdf|work=Manuscript no. nugas1|publisher=Astronomy & Astronophysics|access-date=18 October 2013}}</ref>


==Gallery==
==Gallery==
{{Gallery
<gallery>
|width=176
File:A galaxy with a glowing heart.jpg|NGC 1433 taken by (LEGUS).<ref name=POTW1427a>{{cite news|title=A galaxy with a glowing heart|url=http://www.spacetelescope.org/images/potw1427a/|access-date=8 August 2014|work=ESA/Hubble Picture of the Week}}</ref>
⚫
|File:A galaxy with a glowing heart.jpg|LEGUS, optical.<ref name=POTW1427a>{{cite news|title=A galaxy with a glowing heart|url=http://www.spacetelescope.org/images/potw1427a/|access-date=8 August 2014|work=ESA/Hubble Picture of the Week}}</ref>
File:NGC1433-hst-R814GB450.jpg|[[Hubble Space Telescope|HST]]
|File:NGC1433-hst-R814GB450.jpg|[[Hubble Space Telescope]], optical.
</gallery>
|File:NGC 1433 DSS.jpg|[[Digitized Sky Survey|STSci DSS]], optical.
|File:NGC 1433 (MIRI Image - Annotated) (weic2306b).jpeg|[[James Webb Space Telescope]], [[Mid-Infrared Instrument|MIRI]]; compass. <!-- weic2306b -->
}}


==References==
==References==
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[[Category:Horologium (constellation)]]
[[Category:Horologium (constellation)]]
[[Category:Barred spiral galaxies]]
[[Category:Barred spiral galaxies]]
[[Category:Dorado Group]]
[[Category:Principal Galaxies Catalogue objects|013586]]




Latest revision as of 05:40, 6 December 2024

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 (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]

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]

One supernova has been observed in NGC 1433. SN 1985P (type II, mag. 13.5) was discovered by Robert Evans on 10 October 1985.[9][10][11]

NGC 1433 is member of the Dorado Group.[4][12]

[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. ^ 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. ^ a b "A galaxy with a glowing heart". ESA/Hubble Picture of the Week. Retrieved 8 August 2014.
  9. ^ Evans, R. O.; Thompson, G. (1985). "Supernova 1985P in NGC 1433". International Astronomical Union Circular (4119): 2. Bibcode:1985IAUC.4119....2E.
  10. ^ 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.
  11. ^ "SN 1985P". Transient Name Server. IAU. Retrieved 5 December 2024.
  12. ^ "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.
[edit]
  • Media related to NGC 1433 at Wikimedia Commons


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