NGC 3313

Last updated
NGC 3313
NGC 3313 PanS.jpg
Pan-STARRS image of NGC 3313
Observation data (J2000 epoch)
Constellation Hydra
Right ascension 10h 37m 25.4s [1]
Declination −25° 19′ 10″ [1]
Redshift 0.012362 [1]
Helio radial velocity 3706 km/s [1]
Distance 55.4  Mpc (181  Mly) [1]
Group or cluster Hydra Cluster
Apparent magnitude  (V)12.38 [1]
Characteristics
Type (R')SB(rs)ab [1]
Size~39.04  kpc (127,300  ly) (estimated) [1]
Apparent size  (V)3.9 × 3.2 [1]
Other designations
ESO 501-50, AM 1035-250, IRAS 10350-2503, MCG -4-25-44, PGC 31551, UGCA 213 [1]

NGC 3313 is a large barred spiral galaxy [2] [3] located about 55 megaparsecs (180 million light-years) away in the constellation Hydra. [4] It was discovered by astronomer Ormond Stone in 1886 [5] [6] and is an outlying member of the Hydra Cluster. [7]

Contents

Physical characteristics

NGC 3313 has a complete inner ring feature that is elongated along the bar axis of the galaxy. Inside the inner ring, there are two weak dust lanes in the bar, and surrounding the nucleus there is a very circular nuclear ring. Spiral structure breaking off from the ring region has a complex structure and is tightly wrapped around the ring. The arms trail out into the outer disk where they form a well-defined two-armed pattern. The two-armed pattern also appears to take the form of an R1' outer pseudoring. Beyond this two-armed pattern, there are numerous spiral segments which extend to much larger distances. [3]

One supernova has been observed in NGC 3313: SN 2002jp (type Ic, mag. 16.9). [8]

See also

Related Research Articles

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<span class="mw-page-title-main">ESO 269-57</span> Large spiral galaxy in the constellation Centaurus

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<span class="mw-page-title-main">NGC 521</span> Spiral galaxy in the constellation Cetus

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<span class="mw-page-title-main">NGC 3285</span> Galaxy in the constellation Hydra

NGC 3285 is a barred spiral galaxy located about 200 million light-years away in the constellation Hydra. The galaxy was discovered by astronomer John Herschel on March 24, 1835. NGC 3285 is a member of the Hydra Cluster.

<span class="mw-page-title-main">NGC 3305</span> Galaxy in the constellation Hydra

NGC 3305 is an elliptical galaxy located about 190 million light-years away in the constellation Hydra. The galaxy was discovered by astronomer John Herschel on March 24, 1835. NGC 3305 is a member of the Hydra Cluster.

<span class="mw-page-title-main">NGC 3307</span> Lenticular galaxy in the constellation Hydra

NGC 3307 is a lenticular galaxy located about 185 million light-years away in the constellation Hydra. The galaxy was discovered by astronomer John Herschel on March 22, 1836 and is a member of the Hydra Cluster.

<span class="mw-page-title-main">NGC 3308</span> Lenticular galaxy in the constellation Hydra

NGC 3308 is a lenticular galaxy with a faint bar located about 174 million light-years away in the constellation Hydra. NGC 3308 was discovered by astronomer John Herschel on March 24, 1835. It is a member of the Hydra Cluster.

<span class="mw-page-title-main">NGC 3309</span> Galaxy in the constellation Hydra

NGC 3309 is a giant elliptical galaxy located about 200 million light-years away in the constellation Hydra. NGC 3309 was discovered by astronomer John Herschel on March 24, 1835. The galaxy forms a pair with NGC 3311 which lies about 72,000 ly (22 kpc) away. Both galaxies dominate the center of the Hydra Cluster.

<span class="mw-page-title-main">NGC 3311</span> Galaxy in the constellation Hydra

NGC 3311 is a supergiant elliptical galaxy located about 190 million light-years away in the constellation Hydra. The galaxy was discovered by astronomer John Herschel on March 30, 1835. NGC 3311 is the brightest member of the Hydra Cluster and forms a pair with NGC 3309 which along with NGC 3311, dominate the central region of the Hydra Cluster.

<span class="mw-page-title-main">NGC 3312</span> Spiral galaxy in the constellation Hydra

NGC 3312 is a large and highly inclined spiral galaxy located about 194 million light-years away in the constellation Hydra. The galaxy was discovered by astronomer John Herschel on March 26, 1835. It was later rediscovered by astronomer Guillaume Bigourdan on February 26, 1887. NGC 3312 was later listed and equated with IC 629 because the two objects share essentially the same celestial coordinates. NGC 3312 is the largest spiral galaxy in the Hydra Cluster and is also classified as a LINER galaxy.

<span class="mw-page-title-main">NGC 3315</span> Lenticular galaxy in the constellation Hydra

NGC 3315 is a lenticular galaxy located about 185 million light-years away in the constellation Hydra. It was discovered by astronomer Edward Austin on March 24, 1870. It is a member of the Hydra Cluster.

<span class="mw-page-title-main">NGC 3316</span> Barred lenticular galaxy in the constellation Hydra

NGC 3316 is a barred lenticular galaxy located about 190 million light-years away in the constellation Hydra. The galaxy was discovered by astronomer John Herschel on March 26, 1835. NGC 3316 is a member of the Hydra Cluster, and appears to have a small companion galaxy known as HCC 15.

<span class="mw-page-title-main">NGC 3336</span> Galaxy in the constellation Hydra

NGC 3336 is a barred spiral galaxy located about 190 million light-years away in the constellation Hydra. It was discovered by astronomer John Herschel on March 24, 1835. NGC 3336 is a member of the Hydra Cluster.

<span class="mw-page-title-main">NGC 3369</span> Lenticular galaxy in the constellation Hydra

NGC 3369 is a lenticular galaxy located about 175 million light-years away in the constellation Hydra. NGC 3369 was discovered by astronomer Ormond Stone in 1886 and is an outlying member of the Hydra Cluster.

<span class="mw-page-title-main">NGC 1268</span> Spiral galaxy in the constellation Perseus

NGC 1268 is a spiral galaxy located about 140 million light-years away in the constellation Perseus. It was discovered by astronomer Heinrich d'Arrest on February 14, 1863. NGC 1268 is a member of the Perseus Cluster and appears to show signs of distortion in the form of bridges. These features may be the result of a strong interaction with NGC 1267.

<span class="mw-page-title-main">NGC 3821</span> Spiral galaxy in the constellation Leo

NGC 3821 is a low surface brightness spiral galaxy and a ring galaxy about 270 million light-years away in the constellation Leo. The galaxy was discovered by astronomer William Herschel on April 26, 1785 and is a member of the Leo Cluster.

<span class="mw-page-title-main">NGC 3883</span> Galaxy in the constellation Leo

NGC 3883 is a large low surface brightness spiral galaxy located about 330 million light-years away in the constellation Leo. NGC 3883 has a prominent bulge but does not host an AGN. The galaxy also has flocculent spiral arms in its disk. It was discovered by astronomer William Herschel on April 13, 1785 and is a member of the Leo Cluster.

References

  1. 1 2 3 4 5 6 7 8 9 10 "NASA/IPAC Extragalactic Database". Results for NGC 3313. Retrieved 2018-06-06.
  2. ↑ "Your NED Search Results". ned.ipac.caltech.edu. Retrieved 2018-06-06.
  3. 1 2 "NGC 3313 - SB(r)b". The De Vaucouleurs Atlas of Galaxies. 2017. Retrieved 2018-06-06.
  4. ↑ "Revised NGC Data for NGC 3313". spider.seds.org. Retrieved 2018-06-06.
  5. ↑ Gottlieb, Steve. "Astronomy-Mall: Adventures In Deep Space NGC objects 3001-3999". Astronomy-Mall. Retrieved 2018-04-27.
  6. ↑ "New General Catalog Objects: NGC 3300 - 3349". cseligman.com. Retrieved 2018-05-04.
  7. ↑ Richter, O.-G. (February 1989). "The Hydra I cluster of galaxies. V - A catalogue of galaxies in the cluster area". Astronomy and Astrophysics Supplement Series. 77: 237–256. Bibcode:1989A&AS...77..237R.
  8. ↑ Transient Name Server entry for SN 2002jp. Retrieved 2 April 2023.


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