NGC 7499

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NGC 7499
NGC 7499 NGC 7501 NGC 7503 legacy dr10.jpg
From right to left: NGC 7499, NGC 7501 and NGC 7503
Observation data (J2000 epoch)
Constellation Pisces
Right ascension 23h 10m 22.375s [1]
Declination +07° 34′ 50.20″ [1]
Redshift 0.03947 [2]
Heliocentric radial velocity 11600 km/s [2]
Distance 546.8 ± 38.3  Mly (167.64 ± 11.75  Mpc) [3]
Apparent magnitude  (V)12.98 [4]
Apparent magnitude  (B)14.13 [4]
Characteristics
Type SA00(s): [3]
Other designations
UGC 12397, MCG +01-59-005, PGC 70608 [2]

NGC 7499 is an unbarred lenticular galaxy [3] within the constellation Pisces. NGC 7499 is its New General Catalogue designation. It was discovered on September 2, 1864 by the astronomer Albert Marth. [5]

On 7 December 1986, a supernova was discovered within NGC 7499 and was subsequently designated SN 1986M (type Ib, mag. 16.5). [6] [7]

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<span class="mw-page-title-main">NGC 4780</span> Spiral galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 42</span> Galaxy located in the constellation Pegasus

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<span class="mw-page-title-main">NGC 3258</span> Galaxy in the constellation Antlia

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<span class="mw-page-title-main">NGC 6850</span> Galaxy in the constellation Telescopium

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<span class="mw-page-title-main">NGC 4866</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 3359</span> Galaxy in the constellation Ursa Major

NGC 3359 is a barred spiral galaxy located 59 million light-years from Earth, in the constellation of Ursa Major. It was discovered on November 28, 1793, by the astronomer William Herschel. The central bar is approximately 500 million years old.

<span class="mw-page-title-main">NGC 113</span> Galaxy in the constellation Cetus

NGC 113 is an unbarred lenticular galaxy located in the constellation Cetus. It was discovered by German astronomer, Ernst Wilhelm Leberecht Tempel, on August 27, 1876.

<span class="mw-page-title-main">NGC 124</span> Spiral galaxy in the constellation Cetus

NGC 124 is a spiral galaxy in the constellation Cetus. It was discovered by Truman Henry Safford on September 23, 1867. The galaxy was described as "very faint, large, diffuse, 2 faint stars to northwest" by John Louis Emil Dreyer, the compiler of the New General Catalogue.

<span class="mw-page-title-main">NGC 5470</span> Spiral galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 1573</span> Elliptical galaxy in the constellation Camelopardalis

NGC 1573 is an elliptical galaxy in the constellation of Camelopardalis. It was discovered on 1 August 1883 by Wilhelm Tempel. It was described as "very faint, small" by John Louis Emil Dreyer, the compiler of the New General Catalogue. It is located about 190 million light-years away.

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<span class="mw-page-title-main">NGC 3697</span> Spiral galaxy in the constellation Leo

NGC 3697 is a spiral galaxy in the constellation of Leo. It was discovered on 24 February 1827 by John Herschel. It was described as "extremely faint, very small, extended 90°" by John Louis Emil Dreyer, the compiler of the New General Catalogue. It is a member of HCG 53, a compact group of galaxies.

<span class="mw-page-title-main">NGC 2227</span> Galaxy in the constellation Canis Major

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<span class="mw-page-title-main">NGC 644</span> Galaxy in the constellation of Phoenix

NGC 644 is a barred spiral galaxy in the constellation Phoenix in the southern sky. It is estimated to be 270 million light-years from the Milky Way and has a diameter of approximately 130,000 light-years. Together with NGC 641, it probably forms a gravitationally bound pair of galaxies. The object was discovered on September 5, 1834 by John Herschel.

<span class="mw-page-title-main">NGC 3613</span> Elliptical galaxy in the constellation Ursa Major

NGC 3613 is an elliptical galaxy in the constellation Ursa Major. It was discovered by the astronomer William Herschel on April 8, 1793. NGC 3613 is the center of a cluster of galaxies, and has an estimated globular cluster population of over 2,000.

<span class="mw-page-title-main">NGC 3254</span> Spiral galaxy in the constellation Leo Minor

NGC 3254 is a spiral galaxy in the constellation Leo Minor. It was discovered on March 13, 1785, by the astronomer William Herschel. It is a member of the NGC 3254 Group of galaxies, which is a member of the Leo II Groups, a series of galaxies and galaxy clusters strung out from the right edge of the Virgo Supercluster.

References

  1. 1 2 Skrutskie, Michael F.; Cutri, Roc M.; Stiening, Rae; Weinberg, Martin D.; Schneider, Stephen E.; Carpenter, John M.; Beichman, Charles A.; Capps, Richard W.; Chester, Thomas; Elias, Jonathan H.; Huchra, John P.; Liebert, James W.; Lonsdale, Carol J.; Monet, David G.; Price, Stephan; Seitzer, Patrick; Jarrett, Thomas H.; Kirkpatrick, J. Davy; Gizis, John E.; Howard, Elizabeth V.; Evans, Tracey E.; Fowler, John W.; Fullmer, Linda; Hurt, Robert L.; Light, Robert M.; Kopan, Eugene L.; Marsh, Kenneth A.; McCallon, Howard L.; Tam, Robert; Van Dyk, Schuyler D.; Wheelock, Sherry L. (1 February 2006). "The Two Micron All Sky Survey (2MASS)". The Astronomical Journal. 131 (2): 1163–1183. Bibcode:2006AJ....131.1163S. doi: 10.1086/498708 . ISSN   0004-6256. S2CID   18913331.
  2. 1 2 3 "NGC 7499". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2021-02-04.
  3. 1 2 3 "Results for object NGC 7499 (NGC 7499)". NASA/IPAC Extragalactic Database. California Institute of Technology. Retrieved 2021-02-04.
  4. 1 2 "Search specification: NGC 7499". HyperLeda. Université Claude Bernard Lyon 1. Retrieved 2021-02-04.
  5. ↑ Seligman, Courtney. "New General Catalogue objects: NGC 7450 - 7499". cseligman.com. Retrieved 2021-02-04.
  6. ↑ Cappellaro, E.; Rosino, L. (1986). "IAUC 4282: 1986M; N And 1986; GK Per; Corrs". International Astronomical Union Circular (4282): 1. Bibcode:1986IAUC.4282....1C.
  7. ↑ Transient Name Server entry for SN 1986M. Retrieved 17 July 2024.
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