NGC 5861

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NGC 5861
NGC 5861 PanSTARRS1 i.r.g.jpg
NGC 5861 by PanSTARRS
Observation data (J2000 epoch)
Constellation Libra
Right ascension 15h 09m 16.1s [1]
Declination −11° 19 18 [1]
Redshift 1851 ± 1 km/s [1]
Distance 84 Mly (25.9 Mpc) [1]
Apparent magnitude  (V)11.6
Characteristics
Type SAB(rs)c [1]
Apparent size  (V)3.0 × 1.7 [1]
Other designations
MCG -02-39-003, IRAS 15065-1107, PGC 54097 [1]

NGC 5861 is an intermediate spiral galaxy in constellation Libra. It is located at a distance of about 85 million light years from Earth, which, given its apparent dimensions, means that NGC 5861 is about 80,000 light years across.

Contents

Center image by Hubble Space Telescope NGC5861 - HST - Potw2019a.tif
Center image by Hubble Space Telescope

The galaxy features two long spiral arms that dominate the optical disk. [2] The one arm can be traced from its beginning at the center for nearly one and a half revolutions without branching, whereas the other starts to form fragments after one revolution, forming a moderately chaotic pattern. [3] The galaxy hosts a hydroxyl megamaser. [4]

NGC 5861 is the foremost member of a small galaxy group that also includes NGC 5858, which lies 9.6 arcmin north, forming a non-interactive pair. [5] It is located within the same galaxy cloud with NGC 5878. [6]

Supernovae

Two supernovae have been observed in NGC 5861:

Related Research Articles

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<span class="mw-page-title-main">NGC 7331</span> Galaxy in the constellation Pegasus

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<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 1448</span> Galaxy in the constellation Horologium

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<span class="mw-page-title-main">NGC 4699</span> Spiral galaxy in the constellation Virgo

NGC 4699 is an intermediate spiral galaxy located in the constellation Virgo. It is located at a distance of about 65 million light years from Earth, which, given its apparent dimensions, means that NGC 4699 is about 85,000 light years across. It was discovered by William Herschel in 1786. It is a member of the NGC 4699 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.

<span class="mw-page-title-main">NGC 3631</span> Galaxy in the constellation Ursa Major

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<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 3810</span> Spiral galaxy in the constellation Leo

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<span class="mw-page-title-main">NGC 2280</span> Spiral galaxy in the constellation Canis Major

NGC 2280 is a spiral galaxy located in the constellation Canis Major. It is located at a distance of about 75 million light years from Earth, which, given its apparent dimensions, means that NGC 2280 is about 135,000 light years across. It was discovered by John Herschel on February 1, 1835.

<span class="mw-page-title-main">NGC 7606</span> Galaxy in the constellation Aquarius

NGC 7606 is a spiral galaxy located in the constellation Aquarius. It is located at a distance of circa 100 million light years from Earth, which, given its apparent dimensions, means that NGC 7606 is about 165,000 light years across. It was discovered by William Herschel on September 28, 1785. The galaxy is included in the Herschel 400 Catalogue. It lies 45 arcminutes northeast from psi2 Aquarii. It can be seen with a 4 inch telescope but its visibility is greatly affected by light pollution.

<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

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<span class="mw-page-title-main">NGC 6902</span> Unbarred spiral galaxy in the constellation Sagittarius

NGC 6902 is an unbarred spiral galaxy located in the southern constellation of Sagittarius at an approximate distance of 124 million light-years (38.0 Mpc). NGC 6902 was discovered on September 2, 1836 by English astronomer John Herschel. In his New General Catalogue, Danish astronomer J. L. E. Dreyer described it as faint, considerably small, round, brighter middle. It is a member of the small NGC 6092 group of galaxies; the LGG 434 group.

<span class="mw-page-title-main">NGC 1325</span> Galaxy in the constellation Eridanus

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References

  1. 1 2 3 4 5 6 7 "NASA/IPAC Extragalactic Database". Results for NGC 5861. Retrieved 2016-01-18.
  2. Block, David L.; Puerari, Ivânio; Stockton, Alan; Ferreira, Dewet (6 December 2012). Toward a New Millennium in Galaxy Morphology: From z=0 to the Lyman Break. Springer. p. 16. ISBN   978-9401141147.
  3. Sandage, A.; Bedke, J. (1994). The Carnegie Atlas of Galaxies. Volume I. Carnegie Institution of Washington.
  4. Darling, Jeremy; Giovanelli, Riccardo (July 2002). "A Search for OH Megamasers at z > 0.1. III. The Complete Survey". The Astrophysical Journal. 124 (1): 100–126. arXiv: astro-ph/0205185 . Bibcode:2002AJ....124..100D. doi:10.1086/341166. S2CID   7340232.
  5. de Vaucouleurs, G., de Vaucouleurs, A., and Corwin, H.G. (1976). Second Reference Catalogue of Bright Galaxies. Austin: University of Texas Press.{{cite book}}: CS1 maint: multiple names: authors list (link)
  6. Makarov, Dmitry; Karachentsev, Igor (21 April 2011). "Galaxy groups and clouds in the local (z~ 0.01) Universe". Monthly Notices of the Royal Astronomical Society. 412 (4): 2498–2520. arXiv: 1011.6277 . Bibcode:2011MNRAS.412.2498M. doi: 10.1111/j.1365-2966.2010.18071.x . S2CID   119194025.
  7. "SN 1971D". Transient Name Server. IAU . Retrieved 2 December 2024.
  8. Boffi, F. R.; Sparks, W. B.; Macchetto, F. D. (15 August 1999). "A search for candidate light echoes: Photometry ofsupernova environments". Astronomy and Astrophysics Supplement Series. 138 (2): 253–266. arXiv: astro-ph/9906206 . Bibcode:1999A&AS..138..253B. doi:10.1051/aas:1999274. S2CID   17688690 . Retrieved 29 June 2017.
  9. "SN 2017erp". Transient Name Server. IAU . Retrieved 2 December 2024.