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NGC 1300

Coordinates: Sky map 03h 19m 41.0253s, −19° 24′ 40.149″
From Wikipedia, the free encyclopedia
(Redirected from UGCA 66)
NGC 1300
NGC 1300 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationEridanus
Right ascension03h 19m 41.0253s (49.920939)[1]
Declination−19° 24′ 40.149″ (−19.411153)[1]
Redshift0.005260 (1577 ± 4 km/s)[1]
Distance61.3 Mly (18.8 Mpc)[2]
Apparent magnitude (V)11.4[1]
Characteristics
Type(R')SB(s)bc[1]
Size130,000 ly (39.40 kpc) (estimated)[1]
Apparent size (V)6.2′ × 4.1′[1]
Notable featuresHuge bar-shaped core and two spiral arms
Other designations
ESO 547 -G 31, IRAS 03174-1935, UGCA 66, MCG -03-09-018, PGC 12412[1]

NGC 1300 is a barred spiral galaxy located about 69 million light-years away in the constellation Eridanus. The galaxy is about 130,000 light-years across. It is a member of the Eridanus Cluster, a cluster of 200 galaxies,[3][4][5] in a subgroup of 2–4 galaxies in the cluster known as the NGC 1300 Group.[6][7][8] It was discovered by British astronomer John Herschel on 11 December 1835.[9]

Nucleus

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In the core of the larger spiral structure of NGC 1300, the nucleus shows a "grand-design" spiral structure that is about 3,300 light-years long. Only galaxies with large-scale bars appear to have these grand-design inner disks — a spiral within a spiral. Models suggest that the gas in a bar can be funneled inwards, and then spiral into the center through the grand-design disk, where it can potentially fuel a central supermassive black hole (SMBH). NGC 1300 is not known to have an active nucleus, indicating that its central black hole is not accreting matter. The SMBH has a mass of 7.3+6.9
−3.5×107 M☉.[10][11]

Supernova

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One supernova has been observed in NGC 1300:

  • SN 2022acko (Type II-P, mag. 16.5406) was discovered by the Distance Less Than 40 Mpc Survey (DLT40) on 6 December 2022.[12][13]
Infrared observation of spiral galaxy NGC1300 in the constellation Eridanus.

See also

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References

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  1. 1 2 3 4 5 6 7 8 "NASA/IPAC Extragalactic Database". Results for NGC 1300. Retrieved 2007-03-15.
  2. ↑ Atkinson, J.W.; et al. (2005). "Supermassive black hole mass measurements for NGC 1300 and NGC 2748 based on HST emission-line gas kinematics". Monthly Notices of the Royal Astronomical Society. 359 (2): 504–520. arXiv:astro-ph/0502573. Bibcode:2005MNRAS.359..504A. doi:10.1111/j.1365-2966.2005.08904.x. S2CID 16193663.
  3. ↑ Fouque, P.; Gourgoulhon, E.; Chamaraux, P.; Paturel, G. (1992-05-01). "Groups of galaxies within 80 Mpc. II. The catalogue of groups and group members". Astronomy and Astrophysics Supplement Series. 93: 211–233. Bibcode:1992A&AS...93..211F. ISSN 0365-0138.
  4. ↑ "NGC 1300, a barred spiral galaxy in Eridanus". annesastronomynews.com. 2012-04-27. Retrieved 2013-08-18.
  5. ↑ "The Fornax and Eridanus Clusters". An Atlas of The Universe. Retrieved 2010-05-03.
  6. ↑ Tully, R. Brent (1988). Nearby galaxies catalog. Cambridge; New York: Cambridge University Press. ISBN 978-0-521-35299-4.
  7. ↑ Garcia, A. M. (1993-07-01). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. Bibcode:1993A&AS..100...47G. ISSN 0365-0138.
  8. ↑ Giuricin, Giuliano; Marinoni, Christian; Ceriani, Lorenzo; Pisani, Armando (2000-11-01). "Nearby Optical Galaxies: Selection of the Sample and Identification of Groups". The Astrophysical Journal. 543 (1): 178–194. arXiv:astro-ph/0001140. Bibcode:2000ApJ...543..178G. doi:10.1086/317070. ISSN 0004-637X.
  9. ↑ Seligman, Courtney. "Celestial Atlas: NGC Objects: NGC 1300–1349". cseligman.com. Archived from the original on 12 June 2015. Retrieved 25 July 2015.
  10. ↑ Graham, Alister W. (November 2008). "Populating the Galaxy Velocity Dispersion – Supermassive Black Hole Mass Diagram: A Catalogue of (Mbh, σ) Values". Publications of the Astronomical Society of Australia. 25 (4): 167–175. arXiv:0807.2549. Bibcode:2008PASA...25..167G. doi:10.1071/AS08013. S2CID 89905.
  11. ↑ Atkinson, J. W.; et al. (2005). "Supermassive black hole mass measurements for NGC 1300 and NGC 2748 based on HST emission-line gas kinematics". Monthly Notices of the Royal Astronomical Society. 359 (2): 504–520. arXiv:astro-ph/0502573. Bibcode:2005MNRAS.359..504A. doi:10.1111/j.1365-2966.2005.08904.x. S2CID 16193663.
  12. ↑ "SN 2022acko". Transient Name Server. IAU. Retrieved 10 November 2024.
  13. ↑ Bishop, David. "Supernova 2022acko in NGC 1300". Rochester Astronomy. Retrieved 2023-02-17.
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