| NGC 1380 | |
|---|---|
 NGC 1380 imaged by the Hubble Space Telescope | |
| Observation data (J2000 epoch) | |
| Constellation | Fornax |
| Right ascension | 03h 36m 27.5701s[1] |
| Declination | −34° 58′ 33.721″[1] |
| Redshift | 0.006261 ± 0.000040 [1] |
| Heliocentric radial velocity | 1,877 ± 12 km/s[1] |
| Distance | 60.1 ± 12.1 Mly (18.4 ± 3.7 Mpc)[1] |
| Apparent magnitude (V) | 9.9 |
| Characteristics | |
| Type | SA0 [1] |
| Size | ~139,000 ly (42.63 kpc) (estimated)[1] |
| Apparent size (V) | 4.8′ × 2.3′[1] |
| Other designations | |
| ESO 358- G028, AM 0334-350, IRAS 03345-3508, MCG -06-09-002, PGC 13318[1] | |
NGC 1380 is a lenticular galaxy located in the constellation Fornax. It is located at a distance of about 60 million light years from Earth, which, given its apparent dimensions, means that NGC 1380 is about 85,000 light years across.[1] It was discovered by James Dunlop on September 2, 1826.[2] It is a member of the Fornax Cluster.[3]
Supermassive black hole and nucleus
In the centre of NGC 1380 lies a supermassive black hole whose mass is estimated to be 2.2+1.8
−0.9×108 M☉ based on the velocity dispersion of the globular clusters of the galaxy.[4] The nucleus of NGC 1380 is a probable LINER, based on its narrow emission lines.[5] No broad line region has been detected in NGC 1380. The nuclear spectrum appears reddened, maybe due to the presence of gas and dust around the nucleus, maybe a result of mergers. There appears to be a second element in the nucleus of the galaxy, maybe an HII region.[6] NGC 1380 features a gas disk which co-rotates with the stellar disk, suggesting an internal origin.[5] There is an HII region 1.8 arcseconds south of the nucleus and a diffuse H-alpha region, another HII region, observed 1.8 arcseconds north of the nucleus.[7] The X-ray emission from the galaxy as observed by ROSAT can be explained as thermal emission from a hot interstellar medium and no hard component was detected.[8]
Globular clusters
It is estimated that there are 555±33 globular clusters in NGC 1380. There are two district populations of globular clusters, one red and one blue. The blue globular clusters have similar color and magnitude as the globular clusters in the halo of the Milky Way, but have a flatter surface density profile. The red globular clusters form the majority of the globular clusters of the galaxy. They have similar distribution to the stellar disk of NGC 1380 and have slightly higher metallicity than the globular clusters in the Milky Way, and are associated with the bulge of the galaxy.[9] Based on their size, there are three star cluster populations, the typical globular clusters, with effective radius under 3 pc, the diffuse star clusters, with effective radius circa 5 pc, and the faint fuzzy clusters, with effective radius over 8 pc. The typical globular clusters are closer to the nucleus than the diffuse star clusters.[10]
Environment
NGC 1380 lies in the central part of the Fornax Cluster, 35 arcminutes northwest of the large elliptical galaxy NGC 1399. In the same field of view lie the galaxies NGC 1380A, NGC 1379, NGC 1381, NGC 1382, and NGC 1387. NGC 1380 lies 2 degrees north-northeast of χ2 Fornacis and because of its high surface brightness can be spotted with a five inch telescope even from bright suburban skies.[11]
Based on the properties of its inner stellar halo, it appears that NGC 1380 went through a massive galaxy merger event about 10 billion years ago. The now-consumed satellite galaxy contributed 3.7+2.7
−1.5×1010 M☉ to the mass of NGC 1380, which is about one-fifth of its current mass.[3]
Supernova
One supernova has been detected in NGC 1380: SN 1992A (Type Ia, mag. 12.8) was discovered by W. Liller on 11 January 1992 and independently by N. Brown on 12 January 1992.[12][13]
Gallery
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The central region of NGC 1380, by HST showing a dust disk -
The central part of Fornax Cluster by ESO. NGC 1380 can be seen at the top right of the image.
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See also
References
- ^ a b c d e f g h i j "NASA/IPAC Extragalactic Database". Results for NGC 1380. Retrieved 2016-01-18.
- ^ Seligman, Courtney. "NGC 1380 (= PGC 13419)". Celestial Atlas. Retrieved 19 November 2018.
- ^ a b Zhu, Ling; Van De Ven, Glenn; Leaman, Ryan; Pillepich, Annalisa; Coccato, Lodovico; Ding, Yuchen; Falcón-Barroso, Jesús; Iodice, Enrichetta; Navarro, Ignacio Martin; Pinna, Francesca; Corsini, Enrico Maria; Gadotti, Dimitri A.; Fahrion, Katja; Lyubenova, Mariya; Mao, Shude; McDermid, Richard; Poci, Adriano; Sarzi, Marc; De Zeeuw, Tim (2022). "The Fornax3D project: Discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427". Astronomy & Astrophysics. 664: A115. arXiv:2203.15822. Bibcode:2022A&A...664A.115Z. doi:10.1051/0004-6361/202243109. S2CID 247793082.
- ^ Pota, Vincenzo; Graham, Alister W.; Forbes, Duncan A.; Romanowsky, Aaron J.; Brodie, Jean P.; Strader, Jay (July 2013). "The SLUGGS survey: probing the supermassive black hole connection with bulges and haloes using red and blue globular cluster systems". Monthly Notices of the Royal Astronomical Society. 433 (1): 235–242. arXiv:1304.6723. Bibcode:2013MNRAS.433..235P. doi:10.1093/mnras/stt718. S2CID 35877048.
- ^ a b Ricci, T. V.; Steiner, J. E.; Menezes, R. B. (May 2014). "Integral field unit spectroscopy of 10 early-type galactic nuclei – I. Principal component analysis Tomography and nuclear activity". Monthly Notices of the Royal Astronomical Society. 440 (3): 2419–2441. arXiv:1403.6840. Bibcode:2014MNRAS.440.2419R. doi:10.1093/mnras/stu441. S2CID 118598358.
- ^ Ricci, T. V.; Steiner, J. E.; Menezes, R. B. (May 2014). "IFU spectroscopy of 10 early-type galactic nuclei – II. Nuclear emission line properties". Monthly Notices of the Royal Astronomical Society. 440 (3): 2442–2456. arXiv:1403.6846. Bibcode:2014MNRAS.440.2442R. doi:10.1093/mnras/stu442. S2CID 119255795.
- ^ Ricci, T. V.; Steiner, J. E.; Menezes, R. B. (29 June 2015). "IFU spectroscopy of 10 early-type galactic nuclei – III. Properties of the circumnuclear gas emission". Monthly Notices of the Royal Astronomical Society. 451 (4): 3728–3758. arXiv:1506.03459. Bibcode:2015MNRAS.451.3728R. doi:10.1093/mnras/stv1156. S2CID 118568205.
- ^ Schlegel, Eric M.; Petre, Robert; Loewenstein, Michael (February 1998). "ROSAT Observations of X-Ray–faint S0 Galaxies: NGC 1380". The Astronomical Journal. 115 (2): 525–534. Bibcode:1998AJ....115..525S. doi:10.1086/300217.
- ^ Kissler-Patig, M.; Richtler, T.; Storm, J.; della Valle, M. (1 November 1997). "Halo and bulge/disk globular clusters in the S0 galaxy NGC 1380". Astronomy and Astrophysics. 327: 503–512. arXiv:astro-ph/9706303. Bibcode:1997A&A...327..503K. ISSN 0004-6361.
- ^ Chies-Santos, A. L.; Santiago, B. X.; Pastoriza, M. G. (26 March 2007). "High resolution imaging of the early-type galaxy NGC 1380: an insight into the nature of extended extragalactic star clusters". Astronomy & Astrophysics. 467 (3): 1003–1009. arXiv:astro-ph/0702715. Bibcode:2007A&A...467.1003C. doi:10.1051/0004-6361:20066546. S2CID 17997095.
- ^ O'Meara, Stephen James (2013). Deep-Sky Companions: Southern Gems. Cambridge University Press. pp. 78–80. Bibcode:2013dcsg.book.....O. ISBN 9781107015012.
- ^ Liller, W.; Brown, N.; McNaught, R. H.; Spyromilio, J.; Stathakis, R.; Sadler, E.; Freeman, F.; Cannon, R. (1992). "Supernova 1992A in NGC 1380". International Astronomical Union Circular (5428): 1. Bibcode:1992IAUC.5428....1L.
- ^ "SN 1992A". Transient Name Server. IAU. Retrieved 6 December 2024.
External links
- NGC 1380 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
- NGC 1380 on SIMBAD
