NGC 3313

In today's article we are going to delve into the topic of NGC 3313, an issue that has generated debate and controversy in recent times. NGC 3313 is an issue that affects a wide spectrum of society, from professionals in various areas to ordinary people who face challenges related to this issue in their daily lives. In this article we will explore different perspectives and approaches related to NGC 3313, with the aim of shedding light on its implications and offering a comprehensive view of this issue. Regardless of your level of experience or prior knowledge about NGC 3313, through this article you will find relevant and valuable information that will allow you to better understand this issue and its possible implications in various areas. Read on to delve into the fascinating and complex world of NGC 3313!

NGC 3313
legacy surveys image of NGC 3313
Observation data (J2000 epoch)
ConstellationHydra
Right ascension10h 37m 25.4s[1]
Declination−25° 19′ 10″[1]
Redshift0.012362[1]
Heliocentric radial velocity3706 km/s[1]
Distance55.4 Mpc (181 Mly)[1]
Group or clusterHydra 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]

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

References

  1. ^ a b c d e f g h i j "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. ^ a b "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.