NGC 1448

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NGC 1448
PIA21086 - Galaxy NGC 1448 with Active Galactic Nucleus.jpg
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]

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.

Contents

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. [2]

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. [3]

The galaxy belongs to the NGC 1433 group, [4] part of the Doradus cloud of galaxies.

Supernovae

Six supernovae have been discovered in NGC 1448: SN 1983S (type II, mag. 14.5), [5] SN 2001el (type Ia, mag. 14.5), [6] SN 2003hn (type II, mag. 14.1), [7] SN 2014df (type Ib, mag. 14), [8] SN 2020zbv (type IIP, mag. 18.8), [9] and SN 2021pit (type Ia, mag. 12.3). [10]

Related Research Articles

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<span class="mw-page-title-main">Messier 61</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">Messier 66</span> Intermediate spiral galaxy in the constellation Leo

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<span class="mw-page-title-main">Messier 108</span> Galaxy in the constellation Ursa Major

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<span class="mw-page-title-main">NGC 6745</span> Galaxy in the constellation Lyra

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<span class="mw-page-title-main">NGC 1559</span> Galaxy in the constellation Reticulum

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<span class="mw-page-title-main">Arp 299</span> Pair of galaxies in the constellation Ursa Major

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<span class="mw-page-title-main">Arp 271</span> Interacting galaxies in the constellation Virgo

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<span class="mw-page-title-main">NGC 1084</span> Galaxy in the constellation Eridanus

NGC 1084 is an unbarred spiral galaxy in the constellation Eridanus. It is located at a distance of about 63 million light-years away from the Milky Way. The galaxy was discovered by William Herschel on 10 January 1785. It has multiple spiral arms, which are not well defined. It belongs in the same galaxy group with NGC 988, NGC 991, NGC 1022, NGC 1035, NGC 1042, NGC 1047, NGC 1052 and NGC 1110. This group is in turn associated with the Messier 77 group.

<span class="mw-page-title-main">NGC 908</span> Spiral galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 3464</span> Spiral galaxy in the constellation Hydra

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<span class="mw-page-title-main">NGC 2782</span> Galaxy in the constellation Lynx

NGC 2782 is a peculiar spiral galaxy that formed after a galaxy merger in the constellation Lynx. The galaxy lies 75 million light years away from Earth, which means, given its apparent dimensions, that NGC 2782 is approximately 100,000 light years across. NGC 2782 has an active galactic nucleus and it is a starburst and a type 1 Seyfert galaxy. NGC 2782 is mentioned in the Atlas of Peculiar Galaxies in the category galaxies with adjacent loops.

<span class="mw-page-title-main">NGC 3972</span> Galaxy in the constellation Ursa Major

NGC 3972 is a spiral galaxy located in the northern constellation of Ursa Major. It was discovered by William Herschel on April 14, 1789. This galaxy is located 66 million light years away and is receding with a heliocentric radial velocity of 846 km/s. It is a member of the NGC 3992 Group of galaxies.

<span class="mw-page-title-main">NGC 3147</span> Galaxy in the constellation Draco

NGC 3147 is a spiral galaxy located in the constellation Draco. It is located at a distance of about 130 million light years from Earth, which, given its apparent dimensions, means that NGC 3147 is about 140,000 light years across. It was discovered by William Herschel on April 3, 1785.

<span class="mw-page-title-main">NGC 5018</span> Elliptical galaxy in the constellation Virgo

NGC 5018 is an elliptical galaxy located in the constellation of Virgo at an approximate distance of 132.51 Mly. NGC 5018 was discovered in 1788 by William Herschel.

<span class="mw-page-title-main">NGC 3810</span> Spiral galaxy in the constellation Leo

NGC 3810 is a spiral galaxy located in the constellation Leo. It is about 50 million light years from Earth, and estimated to be about 60,000 light years in diameter. William Herschel discovered it on 15 March 1784.

<span class="mw-page-title-main">NGC 5468</span> Spiral galaxy in the constellation Virgo

NGC 5468 is an intermediate spiral galaxy located in the constellation Virgo. It is located at a distance of about 140 million light-years from Earth, which, given its apparent dimensions, means that NGC 5468 is about 110,000 light-years across. It was discovered by William Herschel on March 5, 1785.

<span class="mw-page-title-main">NGC 7448</span> Galaxy in the constellation of Pegasus

NGC 7448 is a spiral galaxy located in the constellation Pegasus. It is located at a distance of circa 80 million light years from Earth, which, given its apparent dimensions, means that NGC 7448 is about 60,000 light years across. It was discovered by William Herschel on October 16, 1784. It is included in the Atlas of Peculiar Galaxies in the category galaxies with detached segments.

<span class="mw-page-title-main">NGC 4939</span> Spiral galaxy in the constellation Virgo

NGC 4939 is a spiral galaxy located in the constellation Virgo. It is located at a distance of about 120 million light years from Earth, which, given its apparent dimensions, means that NGC 4939 is about 190,000 light years across. It was discovered by William Herschel on March 25, 1786.

<span class="mw-page-title-main">NGC 6951</span> Galaxy in the constellation Cepheus

NGC 6951 is a barred spiral galaxy located in constellation Cepheus. It is located at a distance of about 75 million light-years from Earth, which, given its apparent dimensions, means that NGC 6951 is about 100,000 light-years across. It was discovered by Jérôme Eugène Coggia in 1877 and independently by Lewis Swift in 1878.

References

  1. 1 2 3 4 5 6 7 "NASA/IPAC Extragalactic Database". Results for NGC 1448. Retrieved 2016-01-18.
  2. 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.
  3. Two monster black holes found lurking in nearby galaxies
  4. 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.
  5. Transient Name Server entry for SN 1983S. Retrieved 25 March 2023.
  6. Transient Name Server entry for SN 2001el. Retrieved 25 March 2023.
  7. Transient Name Server entry for SN 2003hn. Retrieved 25 March 2023.
  8. Transient Name Server entry for SN 2014df. Retrieved 25 March 2023.
  9. Transient Name Server entry for SN 2020zbv. Retrieved 25 March 2023.
  10. List of Supernovae IAU Central Bureau for Astronomical Telegrams. Retrieved 29 December 2015.
  11. "Seeing things sideways". www.spacetelescope.org. Retrieved 13 March 2017.