NGC 4580

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NGC 4580
NGC 4580 SDSS.jpeg
SDSS image of NGC 4580
Observation data (J2000 epoch)
Constellation Virgo
Right ascension 12h 37m 48.4s [1]
Declination 05° 22′ 07″ [1]
Redshift 0.003449 [1]
Helio radial velocity 1034 km/s [1]
Distance 69.35  Mly (21.263  Mpc) [1]
Group or cluster Virgo Cluster
Apparent magnitude  (V)12.7 [1]
Characteristics
Type SAB(rs)a pec, LINER [1]
Size~52,400  ly (16.08  kpc) (estimated) [1]
Apparent size  (V)2.28 x 1.45 [1]
Other designations
CGCG 42-183, IRAS 12352+0538, MCG 1-32-117, PGC 42174, UGC 7794, VCC 1730 [1]

NGC 4580 is an unbarred spiral galaxy [2] located about 70 million light-years away [3] in the constellation Virgo. [4] NGC 4580 is also classified as a LINER galaxy. [3] [5] It was discovered by astronomer William Herschel on February 2, 1786 [6] and is a member of the Virgo Cluster. [2] [7]

Contents

Physical characteristics

NGC 4580 consists of a ringed structure. The inner pseudoring of the galaxy is very well-defined and is made of two tightly wound spiral arms. Three very diffuse spiral arms which are partly defined by dust, split off from the inner pseudoring. [2]

Truncated disk

NGC 4580 has a severely truncated star-forming disk. This may be due to ram-pressure stripping [2] caused by the infall of the Messier 49 subcluster into the Virgo Cluster. [8] Due to the truncation of the star forming disk, NGC 4580 is classified as an anemic galaxy. [9]

See also

Related Research Articles

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<span class="mw-page-title-main">Messier 86</span> Elliptical galaxy in the constellation Virgo

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<span class="mw-page-title-main">Messier 90</span> Galaxy in the constellation Virgo

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<span class="mw-page-title-main">NGC 4450</span> Spiral galaxy in the constellation Coma Berenices

NGC 4450 is a spiral galaxy in the constellation Coma Berenices.

<span class="mw-page-title-main">NGC 4323</span> Galaxy in the constellation Coma Berenices

NGC 4323 is a lenticular or dwarf elliptical galaxy located about 52.5 million light-years away in the constellation Coma Berenices. The galaxy was discovered in 1882 by astronomer Wilhelm Tempel and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4651</span> Spiral galaxy in the constellation Coma Berenices

NGC 4651 is a spiral galaxy located in the constellation of Coma Berenices that can be seen with amateur telescopes, at a distance not well determined that ranges from 35 million light years to 72 million light years.

<span class="mw-page-title-main">NGC 4654</span> Galaxy in the constellation Virgo

NGC 4654 is an intermediate spiral galaxy in the constellation of Virgo at a distance of 55 million light years from the Milky Way that can be spotted with amateur telescopes.

<span class="mw-page-title-main">NGC 4457</span> Galaxy in the constellation of Virgo

NGC 4457 is an intermediate spiral galaxy located about 55 million light-years away in the constellation of Virgo. It is also classified as a LINER galaxy, a class of active galaxy defined by their spectral line emissions. NGC 4457 Is inclined by about 33°. It was discovered by astronomer William Herschel on February 23, 1784. Despite being listed in the Virgo Cluster Catalog as VCC 1145, NGC 4457 is a member of the Virgo II Groups which form an extension of the Virgo cluster.

<span class="mw-page-title-main">NGC 4606</span> Spiral galaxy in the constellation Virgo

NGC 4606 is a spiral galaxy located about 55 million light-years away in the constellation of Virgo. NGC 4606 was discovered by astronomer William Herschel on March 15, 1784. It has a disturbed stellar disk suggesting the actions of gravitational interactions. NGC 4607 may be a possible companion of NGC 4606. However, their redshifts differ by about 600 km/s, making it unlikely that they are a gravitationally bound pair. NGC 4606 is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4522</span> Spiral galaxy in the constellation of Virgo

NGC 4522 is an edge-on spiral galaxy located about 60 million light-years away within the Virgo Cluster in the constellation Virgo. NGC 4522 is losing its molecular gas though ram-pressure stripping as it plows though the cluster at a speed of more than 10 million kilometres per hour. The galaxy was discovered by astronomer John Herschel on January 18, 1828.

<span class="mw-page-title-main">NGC 4586</span> Spiral galaxy in the constellation Virgo

NGC 4586 is a spiral galaxy located about 50 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer William Herschel on February 2, 1786. Although listed in the Virgo Cluster Catalog, NGC 4586 is considered to be a member of the Virgo II Groups which form a southern extension of the Virgo cluster. NGC 4586 is currently in the process of infalling into the Virgo Cluster and is predicted to enter the cluster in about 500 million years.

<span class="mw-page-title-main">NGC 4596</span> Galaxy in the constellation Virgo

NGC 4596 is a barred lenticular galaxy located about 55 million light-years away in the constellation Virgo. NGC 4596 was discovered by astronomer William Herschel on March 15, 1784. NGC 4596 is a member of the Virgo Cluster and has an inclination of about 38°.

<span class="mw-page-title-main">NGC 4607</span> Galaxy in the constellation Virgo

NGC 4607 is an edge-on spiral galaxy located about 56 million light-years away in the constellation Virgo. NGC 4607 was discovered by astronomer R. J. Mitchell on April 24, 1854. The galaxy is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4222</span> Edge-on spiral galaxy in the constellation Coma Berenices

NGC 4222 is an edge-on spiral galaxy located about 60 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 8, 1784 and is often misidentified as IC 3087. NGC 4222 is a member of the Virgo Cluster and is a companion of NGC 4216 which lies about 180,000 ly (56 kpc) away. Despite this, the two galaxies are not interacting.

<span class="mw-page-title-main">NGC 4294</span> Galaxy in the constellation Virgo

NGC 4294 is a barred spiral galaxy with flocculent spiral arms located about 55 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer William Herschel on March 15, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4298</span> Galaxy in the constellation Coma Berenices

NGC 4298 is a flocculent spiral galaxy located about 53 million light-years away in the constellation Coma Berenices. The galaxy was discovered by astronomer William Herschel on April 8, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4299</span> Spiral galaxy in the constellation Virgo

NGC 4299 is a featureless spiral galaxy located about 55 million light-years away in the constellation Virgo. It was discovered by astronomer William Herschel on March 15, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4302</span> Galaxy in the constellation Coma Berenices

NGC 4302 is an edge-on spiral galaxy located about 55 million light-years away in the constellation Coma Berenices. It was discovered by astronomer William Herschel on April 8, 1784 and is a member of the Virgo Cluster.

<span class="mw-page-title-main">NGC 4305</span> Dwarf spiral galaxy in the constellation Virgo

NGC 4305 is a dwarf spiral galaxy located about 100 million light-years away in the constellation Virgo. The galaxy was discovered by astronomer John Herschel on May 2, 1829. Although considered to be a member of the Virgo Cluster, its high radial velocity and blue luminosity suggest it is in fact a background galaxy. The galaxy has a nearby major companion; NGC 4306.

References

  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 4580. Retrieved 2018-02-24.
  2. 1 2 3 4 "NGC 4580 - SA(rs)ab". The de Vaucouleurs Atlas of Galaxies. Retrieved 2018-02-24.
  3. 1 2 "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-02-24.
  4. ↑ "Revised NGC Data for NGC 4580". spider.seds.org. Retrieved 2018-02-24.
  5. ↑ "NGC4580" . Retrieved 2018-02-24.
  6. ↑ "New General Catalog Objects: NGC 4550 - 4599". cseligman.com. Retrieved 2018-02-24.
  7. ↑ "The Virgo Cluster". www.atlasoftheuniverse.com. Retrieved 2018-02-24.
  8. ↑ Cortés, Juan R.; Kenney, Jeffrey D. P.; Hardy, Eduardo (2008). "Distances from Stellar Kinematics for Peculiar Virgo Cluster Spiral Galaxies". The Astrophysical Journal. 683 (1): 78. arXiv: 0803.3638 . Bibcode:2008ApJ...683...78C. doi:10.1086/588604. ISSN   0004-637X. S2CID   14426987.
  9. ↑ Koopmann, Rebecca A.; Kenney, Jeffrey D. P. (2004). "Hα Morphologies and Environmental Effects in Virgo Cluster Spiral Galaxies". The Astrophysical Journal. 613 (2): 866–885. arXiv: astro-ph/0406243 . Bibcode:2004ApJ...613..866K. doi:10.1086/423191. ISSN   0004-637X. S2CID   17519217.


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