NGC 1060

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NGC 1060
NGC1060 - SDSS DR14.jpg
NGC 1060 (SDSS)
Observation data (J2000.0 epoch)
Constellation Triangulum
Right ascension 02h 43m 15.05s [1]
Declination +32° 25′ 29.90″ [1]
Redshift 0.017312 [1]
Heliocentric radial velocity 5190 ± 22 km/s [1]
Distance 256 Mly [1]
Apparent magnitude  (V)12.00 [2]
Apparent magnitude  (B)13.00 [2]
Characteristics
Type S0 [1]
Apparent size  (V)2.3 x 1.7 [1]
Other designations
PGC 10302, MCG 5-7-35, UGC 2191

NGC 1060 is a lenticular galaxy approximately 256 million light-years away from Earth in the constellation of Triangulum. [1] It was discovered by William Herschel on September 12, 1784. [3]

Contents

NGC 1060 is the brightest member of the galaxy group LGG 72, which contains approximately 15 galaxies. [4] [5] Intergalactic medium (IGM) in this system is highly disturbed, with separate X-ray peaks centred on the two main galaxies of the group, NGC 1060 and NGC 1066. [4] A ~250 kpc arc of hot gas is linking these two galaxies. [4] The system appears to be undergoing a merger, which may have triggered the nuclear activity in NGC 1060. [4] [5]

In 2013 a small-scale (20”/7.4 kpc) jet source was detected in NGC 1060, indicating a remnant of an old, low power outburst. [4] The radio emission which arises from this jet was also detected. [6] [5]

NGC 1060 is an active galaxy, with confirmed active galactic nucleus (AGN). [6]

Supernova SN 2004fd

Supernova SN 2004fd of magnitude 15.70 was detected in NGC 1060 on October 22, 2004. [7] It was discovered by Tom Boles who was using 0.35m Schmidt-Cassegrain telescope during searches for the UK Nova/Supernova Patrol. [7] The supernova was classified as type Ia, and was located very close to the nucleus of its host galaxy (the J2000 epoch celestial coordinates: RA 02h 43m 15.20s, Dec +32° 25′ 26.00″). [8] [1]

See also

Related Research Articles

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<span class="mw-page-title-main">Messier 84</span> Galaxy in the constellation Virgo

Messier 84 or M84, also known as NGC 4374, is a giant elliptical or lenticular galaxy in the constellation Virgo. Charles Messier discovered the object in 1781 in a systematic search for "nebulous objects" in the night sky. It is the 84th object in the Messier Catalogue and in the heavily populated core of the Virgo Cluster of galaxies, part of the local supercluster.

<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 6946</span> Galaxy in the constellations Cepheus & Cygnus

NGC 6946, sometimes referred to as the Fireworks Galaxy, is a face-on intermediate spiral galaxy with a small bright nucleus, whose location in the sky straddles the boundary between the northern constellations of Cepheus and Cygnus. Its distance from Earth is about 25.2 million light-years or 7.72 megaparsecs, similar to the distance of M101 in the constellation Ursa Major. Both were once considered to be part of the Local Group, but are now known to be among the dozen bright spiral galaxies near the Milky Way but beyond the confines of the Local Group. NGC 6946 lies within the Virgo Supercluster.

<span class="mw-page-title-main">NGC 4261</span> Galaxy in the constellation Virgo

NGC 4261 is an elliptical galaxy located around 100 million light-years away in the constellation Virgo. It was discovered April 13, 1784, by the German-born astronomer William Herschel. The galaxy is a member of its own somewhat meager galaxy group known as the NGC 4261 group, which is part of the Virgo Cluster.

<span class="mw-page-title-main">NGC 1808</span> Galaxy in the constellation Columba

NGC 1808 is a barred spiral galaxy located in the southern constellation of Columba, about two degrees to the south and east of Gamma Caeli. It was discovered by Scottish astronomer James Dunlop, who described it as a "faint nebula". The galaxy is a member of the NGC 1808 group, which is part of the larger Dorado Group.

<span class="mw-page-title-main">NGC 4666</span> Spiral galaxy in the constellation Virgo

NGC 4666 is a spiral galaxy in the equatorial constellation of Virgo, located at a distance of approximately 55 megalight-years from the Milky Way. It was discovered by the German-born astronomer William Herschel on February 22, 1784. It is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. John L. E. Dreyer described it as "bright, very large, much extended 45°±, pretty suddenly brighter middle". It is a member of an interacting system with NGC 4668 and a dwarf galaxy, and belongs to a small group that also includes NGC 4632.

<span class="mw-page-title-main">NGC 7552</span> Galaxy in the constellation Grus

NGC 7552 is a barred spiral galaxy in the constellation Grus. It is at a distance of roughly 60 million light years from Earth, which, given its apparent dimensions, means that NGC 7552 is about 75,000 light years across. It forms with three other spiral galaxies the Grus Quartet.

<span class="mw-page-title-main">NGC 4274</span> Galaxy in the constellation Coma Berenices

NGC 4274 is a barred spiral galaxy located in the constellation Coma Berenices. It is located at a distance of circa 45 million light years from Earth, which, given its apparent dimensions, means that NGC 4274 is about 95,000 light years across. It was discovered by William Herschel in 1785.

<span class="mw-page-title-main">NGC 6810</span> Galaxy in the constellation of Pavo

NGC 6810 is a spiral galaxy approximately 87 million light-years away from Earth in the constellation of Pavo.

<span class="mw-page-title-main">NGC 1272</span> Galaxy in the constellation Perseus

NGC 1272 is a massive elliptical galaxy located about 230 million light-years away in the constellation Perseus. It was discovered by astronomer Heinrich d'Arrest on February 14, 1863. NGC 1272 has an active nucleus and is the second brightest member of the Perseus Cluster after NGC 1275.

<span class="mw-page-title-main">NGC 3367</span> Spiral galaxy in the constellation Leo

NGC 3367 is a barred spiral galaxy located in the constellation Leo. It is located at a distance of about 120 million light years from Earth, which, given its apparent dimensions, means that NGC 3367 is about 85,000 light years across. It was discovered by William Herschel on March 19, 1784.

<span class="mw-page-title-main">NGC 1380</span> Galaxy in the constellation Fornax

NGC 1380 is a lenticular galaxy located in the constellation Fornax. It is located at a distance of circa 60 million light years from Earth, which, given its apparent dimensions, means that NGC 1380 is about 85,000 light years across. It was discovered by James Dunlop on September 2, 1826. It is a member of the Fornax Cluster.

<span class="mw-page-title-main">NGC 4636</span> Galaxy in the constellation Virgo

NGC 4636 is an elliptical galaxy located in the constellation Virgo. It is a member of the NGC 4753 Group of galaxies, which is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. It is located at a distance of about 55 million light years from Earth, which, given its apparent dimensions, means that NGC 4636 is about 105,000 light years across.

<span class="mw-page-title-main">NGC 759</span> Galaxy in the constellation Andromeda

NGC 759 is an elliptical galaxy located 230 million light-years away in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865. It is a member of Abell 262.

<span class="mw-page-title-main">NGC 3665</span> Galaxy in the constellation Ursa Major

NGC 3665 is a lenticular galaxy located in the constellation Ursa Major. It is located at a distance of circa 85 million light-years from Earth, which, given its apparent dimensions, means that NGC 3665 is about 85,000 light years across. It was discovered by William Herschel on March 23, 1789.

<span class="mw-page-title-main">NGC 4061</span> Galaxy in the constellation Coma Berenices

NGC 4061 is an elliptical galaxy located 310 light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 27, 1785. It was rediscovered by John Herschel on April 29, 1832. It is listed both as NGC 4061 and NGC 4055. NGC 4061 is a member of the NGC 4065 Group and forms an interacting pair with its companion, NGC 4065 as evidenced by distortions in their optical isophotes.

<span class="mw-page-title-main">NGC 877</span> Galaxy located in the constellation Aries

NGC 877 is an intermediate spiral galaxy located in the constellation Aries. It is located at a distance of circa 160 million light years from Earth, which, given its apparent dimensions, means that NGC 877 is about 115,000 light years across. It was discovered by William Herschel on October 14, 1784. It interacts with NGC 876.

<span class="mw-page-title-main">NGC 765</span> Galaxy in the constellation Aries

NGC 765 is an intermediate spiral galaxy located in the constellation Aries. It is located at a distance of circa 220 million light years from Earth, which, given its apparent dimensions, means that NGC 765 is about 195,000 light years across. It was discovered by Albert Marth on October 8, 1864. The galaxy has an extensive hydrogen (HI) disk with low surface brightness, whose diameter is estimated to be 240 kpc.

<span class="mw-page-title-main">NGC 1106</span> Galaxy in the constellation Perseus

NGC 1106 is a lenticular, non-barred spiral galaxy with considerable structure, located in the Perseus constellation. It was first observed by astronomer John Herschel in 1828.

References

  1. 1 2 3 4 5 6 7 8 9 "NASA/IPAC Extragalactic Database". ned.ipac.caltech.edu. Retrieved December 7, 2017.
  2. 1 2 "Revised NGC Data for NGC 1060". spider.seds.org. Retrieved December 9, 2017.
  3. ↑ "Data for NGC 1060". www.astronomy-mall.com. Retrieved December 9, 2017.
  4. 1 2 3 4 5 Kolokythas, K.; et al. (2014). "Radio properties of nearby groups of galaxies". In Chengalur, J. N. (ed.). Proceedings of the Metrewavelength Sky conference. Astronomical Society of India. arXiv: 1402.5109v1 . Bibcode:2014ASInC..13..197K.
  5. 1 2 3 Vrtilek, Jan M; O'Sullivan, E; David, L. P; Kolokythas, K; Giacintucci, S; Raychaudhury, S; Ponman, T. J (2013). "CLoGS - the Complete Local-Volume Groups Survey". American Astronomical Society. 13: 116.06. Bibcode:2013HEAD...1311606V.
  6. 1 2 O’Sullivan, E.; et al. (2015). "Cold gas in group-dominant elliptical galaxies". Astronomy and Astrophysics . 573: A111. arXiv: 1408.7106 . Bibcode:2015A&A...573A.111O. doi:10.1051/0004-6361/201424835. S2CID   119280629.
  7. 1 2 "THE ASTRONOMER Electronic Circular No 2056". www.theastronomer.org. Retrieved December 7, 2017.
  8. ↑ Boles, T. (2004). "Supernova 2004fd in NGC 1060". IAU Circular. 8423: 1. Bibcode:2004IAUC.8423....1B . Retrieved December 7, 2017.
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