| NGC 1300 | |
|---|---|
 A
Hubble Space Telescope (HST) image of NGC 1300 | |
| Observation data ( J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 19m 41.1s (49.9210) [1] |
| Declination | −19° 24′ 41″ (-19.4112) [1] |
| Redshift | 0.005260 (1577 ± 4 km/ s) [1] |
| Distance | 61.3 Mly (18.8 M pc) [2] |
| Apparent magnitude (V) | 11.4 [1] |
| Characteristics | |
| Type | (R')SB(s)bc [1] |
| Size | 110,000 light years in diameter |
| Apparent size (V) | 6.2′ × 4.1′ [1] |
| Notable features | Huge bar-shaped core and two spiral arms |
| Other designations | |
| MCG-03-09-018,
[1] ESO 547 -G 31,
[1] PGC 12412, [1] UGCA 066 [1] | |
NGC 1300 is a barred spiral galaxy located about 65 million light-years away in the constellation Eridanus. The galaxy is about 110,000 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 John Herschel in 1835. [9]
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]
At least one supernova has been observed in NGC 1300: SN 2022acko (type IIP, mag. 15.8). [12] [13]
- NGC 1672, a similar spiral galaxy
- NGC 7479, a galaxy with a very similar structure and both size and morphology similar
- NGC 1232, a nearby intermediate spiral galaxy
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 1300. Retrieved 2007-03-15.
- ^ 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.
- ^ 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. ISSN 0365-0138.
- ^ "NGC 1300, a barred spiral galaxy in Eridanus". annesastronomynews.com. 2012-04-27. Retrieved 2013-08-18.
- ^ "The Fornax and Eridanus Clusters". An Atlas of The Universe. Retrieved 2010-05-03.
- ^ Tully, R. Brent (1988). Nearby galaxies catalog. Cambridge ; New York: Cambridge University Press. ISBN 978-0-521-35299-4.
- ^ Garcia, A. M. (1993-07-01). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. ISSN 0365-0138.
- ^ 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: 178–194. doi: 10.1086/317070. ISSN 0004-637X.
- ^ Seligman, Courtney. "Celestial Atlas: NGC Objects: NGC 1300 - 1349". cseligman.com. Archived from the original on 12 June 2015. Retrieved 25 July 2015.
- ^ 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.
- ^ 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.
- ^ SN 2022acko Retrieved 29 December 2022.
- ^ David Bishop. "Supernova 2022acko in NGC 1300". Retrieved 2023-02-17.
- HST: Barred Spiral Galaxy NGC 1300
- Hubble Heritage
- NASA Astronomy Picture of the Day: Barred Spiral Galaxy NGC 1300 (12 January 2005)
- NGC 1300 in Eridanus
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| NGC 1300 | |
|---|---|
|
A
Hubble Space Telescope (HST) image of NGC 1300 | |
| Observation data ( J2000 epoch) | |
| Constellation | Eridanus |
| Right ascension | 03h 19m 41.1s (49.9210) [1] |
| Declination | −19° 24′ 41″ (-19.4112) [1] |
| Redshift | 0.005260 (1577 ± 4 km/ s) [1] |
| Distance | 61.3 Mly (18.8 M pc) [2] |
| Apparent magnitude (V) | 11.4 [1] |
| Characteristics | |
| Type | (R')SB(s)bc [1] |
| Size | 110,000 light years in diameter |
| Apparent size (V) | 6.2′ × 4.1′ [1] |
| Notable features | Huge bar-shaped core and two spiral arms |
| Other designations | |
| MCG-03-09-018,
[1] ESO 547 -G 31,
[1] PGC 12412, [1] UGCA 066 [1] | |
NGC 1300 is a barred spiral galaxy located about 65 million light-years away in the constellation Eridanus. The galaxy is about 110,000 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 John Herschel in 1835. [9]
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]
At least one supernova has been observed in NGC 1300: SN 2022acko (type IIP, mag. 15.8). [12] [13]
- NGC 1672, a similar spiral galaxy
- NGC 7479, a galaxy with a very similar structure and both size and morphology similar
- NGC 1232, a nearby intermediate spiral galaxy
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 1300. Retrieved 2007-03-15.
- ^ 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.
- ^ 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. ISSN 0365-0138.
- ^ "NGC 1300, a barred spiral galaxy in Eridanus". annesastronomynews.com. 2012-04-27. Retrieved 2013-08-18.
- ^ "The Fornax and Eridanus Clusters". An Atlas of The Universe. Retrieved 2010-05-03.
- ^ Tully, R. Brent (1988). Nearby galaxies catalog. Cambridge ; New York: Cambridge University Press. ISBN 978-0-521-35299-4.
- ^ Garcia, A. M. (1993-07-01). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47–90. ISSN 0365-0138.
- ^ 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: 178–194. doi: 10.1086/317070. ISSN 0004-637X.
- ^ Seligman, Courtney. "Celestial Atlas: NGC Objects: NGC 1300 - 1349". cseligman.com. Archived from the original on 12 June 2015. Retrieved 25 July 2015.
- ^ 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.
- ^ 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.
- ^ SN 2022acko Retrieved 29 December 2022.
- ^ David Bishop. "Supernova 2022acko in NGC 1300". Retrieved 2023-02-17.
- HST: Barred Spiral Galaxy NGC 1300
- Hubble Heritage
- NASA Astronomy Picture of the Day: Barred Spiral Galaxy NGC 1300 (12 January 2005)
- NGC 1300 in Eridanus
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| Galaxies |
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