NGC 337

NGC 337
A barred spiral galaxy on a dark background. The galaxy’s central region is a pale colour due to older stars, contains some pale reddish threads of dust, and is brighter along a broad horizontal bar through the very centre. Off the bar come several stubby spiral arms, merging into the outer region of the disc. It is a cool blue colour and contains some bright sparkling blue spots, both indicating young hot stars.
NGC 337 imaged by the Hubble Space Telescope
Observation data (J2000 epoch)
ConstellationCetus
Right ascension00h 59m 50.0064s
Declination−07° 34′ 40.94″
Redshift0.005504
Heliocentric radial velocity1650 ± 1 km/s
Distance64.0 ± 4.6 Mly (19.63 ± 1.41 Mpc)
Group or clusterNGC 337 Group (LGG 15)
Apparent magnitude (V)12.46
Characteristics
TypeSB(s)d
Size~60,400 ly (18.52 kpc) (estimated)
Apparent size (V)2.9' × 1.8'
Other designations
IRAS 00573-0750, 2MASX J00595009-0734406, MCG -01-03-053, PGC 3572

NGC 337 is a barred spiral galaxy in the constellation Cetus. Its velocity with respect to the cosmic microwave background is 1,331±22 km/s, which corresponds to a Hubble distance of 64.0 ± 4.6 Mly (19.63 ± 1.41 Mpc). Additionally, 20 non-redshift measurements give a similar distance of 63.11 ± 1.81 Mly (19.350 ± 0.556 Mpc).

It was discovered on September 10, 1785 by German-British astronomer William Herschel. It was described by John Dreyer as "pretty faint, large, extended, gradually a little brighter middle, 10th magnitude star 21 seconds of time to the east."

NGC 337 is considered as a Late-Type Morphology galaxy, with a Star Formation Rate (SFR) of 1.62 M⊙ yr⁻¹ and has a Star Formation Efficiency (sSFR) of -9.62.

Supernovae

Two supernovae have been observed in NGC 337:

NGC 337 Group

NGC 337 is the largest and brightest galaxy in the NGC 337 Group (also known as LGG 15). The group includes at least three other galaxies: NGC 274, NGC 275, and NGC 298.

See also

References

  1. 1 2 3 4 5 6 7 8 9 10 11 "Results for object NGC 0337". NASA/IPAC Extragalactic Database. NASA and Caltech. Retrieved September 2, 2016.
  2. ↑ "Distance Results for NGC 337". NASA/IPAC EXTRAGALACTIC DATABASE. NASA. Retrieved December 19, 2024.
  3. 1 2 Seligman, Courtney. "New General Catalogue Objects: NGC 337". Celestial Atlas. Retrieved December 19, 2024.
  4. ↑ Bitsakis, T.; Charmandaris, V.; Appleton, P. N.; Díaz-Santos, T.; Le Floc'h, E.; da Cunha, E.; Alatalo, K.; Cluver, M. (2014). "Herschel observations of Hickson compact groups of galaxies: Unveiling the properties of cold dust". Astronomy & Astrophysics. 565: A25. arXiv:1402.1470. Bibcode:2014A&A...565A..25B. doi:10.1051/0004-6361/201323349.
  5. ↑ Monard, L. A. G.; Valenti, S.; Benetti, S. (2011). "Supernova 2011dq in NGC 337 = PSN J00594775-0734205". Central Bureau Electronic Telegrams (2749): 1. Bibcode:2011CBET.2749....1M.
  6. ↑ "SN 2011dq". Transient Name Server. IAU. Retrieved December 19, 2024.
  7. ↑ Nakano, S.; Itagaki, K.; Yusa, T.; Howerton, S.; Elias-Rosa, N.; Tartaglia, L.; Cappellaro, E.; Pastorello, A.; Botticella, M. T.; Inserra, C.; Maguire, K.; Smartt, S.; Smith, K. W.; Sullivan, M.; Valenti, S.; Yaron, O.; Young, D.; Manulis, I. (2014). "Supernova 2014cx in NGC 337 = PSN J00594783-0734186". Central Bureau Electronic Telegrams (3963): 1. Bibcode:2014CBET.3963....1N.
  8. ↑ "SN 2014cx". Transient Name Server. IAU. Retrieved December 19, 2024.
  9. ↑ Garcia, A. M. (1993). "General study of group membership. II. Determination of nearby groups". Astronomy and Astrophysics Supplement Series. 100: 47. Bibcode:1993A&AS..100...47G.