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NGC 1448 or NGC 1457 is an unbarred spiral galaxy seen nearly edge-on in the constellation Horologium. It is at a distance of 55 million light years from Earth. It was discovered by John Herschel in 1835. Five supernovae have been discovered in NGC 1448, SN 1983S (14.5 mag, type II), SN 2001el (14.5 mag, type Ia), SN 2003hn (14.1 mag. type II), SN 2014df (14.0 mag., type Ib) and SN 2021pit (12.3 mag. type Ia).[2]
| NGC 1448 | |
|---|---|
 NGC 1448 by NuSTAR and the Chandra X-ray Observatory | |
| Observation data (J2000 epoch) | |
| Constellation | Horologium |
| Right ascension | 03h 44m 31.9s[1] |
| Declination | −44° 38′ 41″[1] |
| Redshift | 1168 ± 2 km/s[1] |
| Distance | 56.5 ± 7.6 Mly (17.3 ± 2.3 Mpc)[1] |
| Apparent magnitude (V) | 10.7 |
| Characteristics | |
| Type | SAcd [1] |
| Apparent size (V) | 7′.6 × 1′.7[1] |
| Other designations | |
| NGC 1457, PGC 13727[1] | |
From the spectral analysis of SN 2001el, over a dozen diffuse interstellar bands were discovered in NGC 1448 – one of the few cases that these bands were observed outside of the Milky Way. However, the bands were significantly weaker at SN 2003hn.[3]
In January 2017 it was announced that evidence for a supermassive black hole in NGC 1448 had been found in the center of the galaxy.[4]
The galaxy belongs to the NGC 1433 group,[5] part of the Doradus cloud of galaxies.
Gallery
![NGC 1448 taken by the Hubble Space Telescope's Wide Field Camera 3.[6]](//upload.wikimedia.org/wikipedia/commons/thumb/d/dd/NGC_1448_Seeing_things_sideways.jpg/120px-NGC_1448_Seeing_things_sideways.jpg)
NGC 1448 taken by the Hubble Space Telescope's Wide Field Camera 3.[6]
![NGC 1448 taken by the Hubble Space Telescope's Wide Field Camera 3.[6]](http://upload.wikimedia.org/wikipedia/commons/d/dd/NGC_1448_Seeing_things_sideways.jpg)
References
- "NASA/IPAC Extragalactic Database". Results for NGC 1448. Retrieved 2016-01-18.
- List of Supernovae IAU Central Bureau for Astronomical Telegrams. Retrieved 29 December 2015.
- J. Sollerman; N. Cox; S. Mattila; P. Ehrenfreund; L. Kaper; B. Leibundgut; P. Lundqvist (January 2005). "Diffuse Interstellar Bands in NGC 1448". Astronomy and Astrophysics. 429 (2): 559–567. arXiv:astro-ph/0409340. Bibcode:2005A&A...429..559S. doi:10.1051/0004-6361:20041465. S2CID 18036448. Retrieved 16 January 2016.
- Two monster black holes found lurking in nearby galaxies
- Dmitry Makarov; Igor Karachentsev (2011). "Galaxy groups and clouds in the local (z∼ 0.01) Universe". MNRAS. 412 (4): 2498–2520. arXiv:1011.6277. Bibcode:2011MNRAS.412.2498M. doi:10.1111/j.1365-2966.2010.18071.x. S2CID 119194025. Retrieved 1 January 2016.
- "Seeing things sideways". www.spacetelescope.org. Retrieved 13 March 2017.
External links
- NGC 1448 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images
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На других языках
[de] NGC 1448
NGC 1448 = NGC 1457 ist eine Spiralgalaxie vom Hubble-Typ Sc[2] im Sternbild Horologium am Südsternhimmel. Sie ist schätzungsweise 46 Millionen Lichtjahre von der Milchstraße entfernt und hat einen Durchmesser von etwa 110.000 Lichtjahren.- [en] NGC 1448
[ru] NGC 1448
NGC 1448 (другие обозначения — NGC 1457, ESO 249-16, MCG −7-8-5, AM 0342-444, PGC 13727) — спиральная галактика (Sc) в созвездии Часы.Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
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