NGC 3583

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NGC 3583
Galaxy galaxy, burning bright! (49869421071).jpg
NGC 3583 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
Constellation Ursa Major
Right ascension 11h 14m 10.9s [1]
Declination 48° 19′ 07″ [1]
Redshift 0.007022 ± 0.000010 [1]
Heliocentric radial velocity 2,105 ± 3 km/s [1]
Distance 90.5 ± 10.2 Mly (27.7 ± 3.1 Mpc) [1]
Apparent magnitude  (V)11.2
Characteristics
Type SB(s)b [1]
Apparent size  (V)3.04′ × 1.16′ [1]
Other designations
UGC 6263, MCG +08-21-008, PGC 34232, 5C 02.203 [1]

NGC 3583 is a barred spiral galaxy located in the constellation Ursa Major. It is located at a distance of circa 90 million light years from Earth, which, given its apparent dimensions, means that NGC 3583 is about 85,000 light years across. It was discovered by William Herschel on February 5, 1788. [2]

Contents

NGC 3585 has a bright nucleus and an elliptical bulge. [3] It has a prominent bar which is about 30 arcseconds long. [4] The spiral arms start approximately at the radius of the end of the bar. One arm emanates from northwest edge of the bulge. At its start is quite diffuse but after passing near the bar becomes better defined. After reaching the southeast part of the galaxy it starts to fade. The other arm emanates from the southeast end of the bar. It appears to branch after passing from the other side of the bar, with the two branches running parallelly. [3]

The galaxy has many HII regions. [4] The star formation rate in the galaxy based on the infrared luminosity is 9.8 M☉ per year. [5]

NGC 3583 is the foremost galaxy in the NGC 3583 galaxy group. Also member of the group is the galaxy NGC 3595, while a bit farther away lies NGC 3614 and its group. [6] NGC 3583 forms a pair with a small elliptical galaxy, which lies 0.9 arcminutes from NGC 3583. Barred spiral galaxy NGC 3577 lies at a projected distance of 5 arcminutes. [7]

Supernovae

Two supernovae have been observed in NGC 3583:

See also

Related Research Articles

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

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<span class="mw-page-title-main">NGC 4725</span> Galaxy in the constellation Coma Berenices

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<span class="mw-page-title-main">NGC 3169</span> Galaxy in the constellation Sextans

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<span class="mw-page-title-main">NGC 5668</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 4041</span> Spiral galaxy in the constellation Ursa Major

NGC 4041 is the New General Catalogue identifier for a spiral galaxy in the northern circumpolar constellation of Ursa Major. It is located an estimated 70 million light years from the Sun. The morphological classification of SA(rs)bc indicates this is a spiral galaxy the lacks a bar; the 'rs' means it has a weakly-formed ring structure, and the 'bc' indicates the spiral arms are moderately to loosely wound.

<span class="mw-page-title-main">NGC 4178</span> Galaxy in the constellation Virgo

NGC 4178 is the New General Catalogue identifier for a barred spiral galaxy in the equatorial constellation of Virgo. It was discovered April 11, 1825 by English astronomer John Herschel. Located some 43.8 million light years away, this galaxy spans 2.3 × 0.4 arc minutes and is seen at a low angle, being inclined by 77° to the line of sight from the Earth. The morphological classification of NGC 4178 is SB(rs)dm, indicating that it has a bar feature at the core, and, per the '(rs)', has traces of a ring-like structure surrounding the bar. The 'dm' suffix indicates the spiral arms are diffuse, broken, and irregular in appearance with no bulge at the nucleus. This galaxy is a member of the Virgo Cluster, which is the richest nearby group of galaxies outside the Local Group and forms the core of the Virgo Supercluster.

<span class="mw-page-title-main">ASASSN-15lh</span> 2015 hypernova event in the constellation Indus

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<span class="mw-page-title-main">NGC 3191</span> Galaxy in the constellation Ursa Major

NGC 3191 is a barred spiral galaxy in the constellation Ursa Major. It was discovered on 5 February 1788 by William Herschel. It is located at a distance of about 400 million light years from Earth, which, given its apparent dimensions, means that NGC 3191 is about 115,000 light years across.

<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 2336</span> Galaxy in the constellation Camelopardalis

NGC 2336 is a barred spiral galaxy located in the constellation Camelopardalis. It is located at a distance of circa 100 million light years from Earth, which, given its apparent dimensions, means that NGC 2336 is about 200,000 light years across. It was discovered by Wilhelm Tempel in 1876.

<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 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 7130</span> Galaxy in the constellation Piscis Austrinus

NGC 7130 is a spiral galaxy located in the constellation Piscis Austrinus. It is located at a distance of about 220 million light years from Earth, which, given its apparent dimensions, means that NGC 7130 is about 100,000 light years across. It was discovered by John Herschel on September 25, 1834, and discovered independently by Lewis Swift on September 17, 1897. The location of the galaxy given in the New General Catalogue was off by 30 arcminutes in declination from the location of the galaxy.

<span class="mw-page-title-main">NGC 7418</span> Galaxy in the constellation Grus

NGC 7418 is an intermediate spiral galaxy located in the constellation Grus. It is located at a distance of circa 60 million light-years from Earth, which, given its apparent dimensions, means that NGC 7418 is about 60,000 light-years across. It was discovered by John Herschel on August 30, 1834.

<span class="mw-page-title-main">NGC 5728</span> Spiral galaxy in the constellation Libra

NGC 5728 is an active barred spiral galaxy located 146 million light years away in the southern constellation of Libra. It was discovered on May 7, 1787 by William Herschel. The designation comes from the New General Catalogue of J. L. E. Dreyer, published in 1888. It has an apparent visual magnitude of 13.40 and spans an angle of 3.4 arcminutes. The galaxy shows a red shift of 0.00935 and has a heliocentric radial velocity of 2,803 km/s. It has an estimated mass of 72 billion times the mass of the Sun and stretches around 30 kpc across.

<span class="mw-page-title-main">NGC 5135</span> Galaxy in the constellation Hydra

NGC 5135 is a barred spiral galaxy located in the constellation Hydra. It is located at a distance of about 200 million light years from Earth. It was discovered by John Herschel on May 8, 1834. It is a Seyfert galaxy.

<span class="mw-page-title-main">NGC 5996</span> Spiral galaxy in the constellation Serpens

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References

  1. 1 2 3 4 5 6 7 8 "NASA/IPAC Extragalactic Database". Results for NGC 3583. Retrieved 2023-07-04.
  2. ↑ Seligman, Courtney. "NGC 3583". Celestial Atlas. Retrieved 19 November 2018.
  3. 1 2 Eskridge, Paul B.; Frogel, Jay A.; Pogge, Richard W.; Quillen, Alice C.; Berlind, Andreas A.; Davies, Roger L.; DePoy, D. L.; Gilbert, Karoline M.; Houdashelt, Mark L.; Kuchinski, Leslie E.; Ramirez, Solange V.; Sellgren, K.; Stutz, Amelia; Terndrup, Donald M.; Tiede, Glenn P. (November 2002). "Near-Infrared and Optical Morphology of Spiral Galaxies". The Astrophysical Journal Supplement Series. 143 (1): 73–111. arXiv: astro-ph/0206320 . Bibcode:2002ApJS..143...73E. doi:10.1086/342340. S2CID   15491635.
  4. 1 2 Fridman, A. M.; Afanasiev, V. L.; Dodonov, S. N.; Khoruzhii, O. V.; Moiseev, A. V.; Sil'chenko, O. K.; Zasov, A. V. (January 2005). "The orientation parameters and rotation curves of 15 spiral galaxies". Astronomy & Astrophysics. 430 (1): 67–81. arXiv: astro-ph/0409622 . Bibcode:2005A&A...430...67F. doi: 10.1051/0004-6361:200400087 . S2CID   39130734.
  5. ↑ Misiriotis, A.; Papadakis, I. E.; Kylafis, N. D.; Papamastorakis, J. (April 2004). "Dust masses and star formation in bright IRAS galaxies: Application of a physical model for the interpretation of FIR observations". Astronomy & Astrophysics. 417 (1): 39–50. arXiv: astro-ph/0312258 . Bibcode:2004A&A...417...39M. doi: 10.1051/0004-6361:20035602 . S2CID   17851708.
  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. ↑ de Vaucouleurs, G.; de Vaucouleurs, A.; Corwin, J. R. (1 January 1976). "Second reference catalogue of bright galaxies". Second Reference Catalogue of Bright Galaxies. 1976. Bibcode:1976RC2...C......0D.
  8. ↑ Kowal, C. (1975). "Supernova in NGC 3583". International Astronomical Union Circular (2878): 1. Bibcode:1975IAUC.2878....1K.
  9. ↑ "SN 1975P". Transient Name Server. IAU . Retrieved 3 December 2024.
  10. ↑ Stanek, K. Z.; Kochanek, C. S.; Brown, J. S.; Holoien, T. W. -S.; Godoy-Rivera, D.; Basu, U.; Shappee, B. J.; Prieto, J. L.; Bersier, D.; Dong, Subo; Chen, Ping; Brimacombe, J.; Kiyota, S.; Masi, G.; Nicholls, B. (2015). "ASASSN-15so: Discovery of a Bright Probable Supernova in NGC 3583". The Astronomer's Telegram. 8256: 1. Bibcode:2015ATel.8256....1S.
  11. ↑ Zhang, Xiliang; Zhang, Jujia; Dong, Subo; Stanek, K. Z. (1 November 2015). "Spectroscopic Classification of ASASSN-15so as a young Type Ia Supernova". The Astronomer's Telegram. 8261: 1. Bibcode:2015ATel.8261....1Z.
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