NGC 428

NGC 428

Hubble image of NGC 428.
Observation data (J2000.0 epoch)
Constellation Cetus[1]
Distance 48 mly [2]

NGC 428 is a barred spiral galaxy in the constellation of Cetus (The Sea Monster), with its spiral structure distorted and warped, possibly the result of the collision of two galaxies.[2] There appears to be a substantial amount of star formation occurring within NGC 428 — a telltale sign of a galaxy merger.[2] In 2015 the Hubble Space Telescope made a close-up shot of the galaxy with its Advanced Camera for Surveys and its Wide Field and Planetary Camera 2.[1] The structure of NGC 428 has been compared to NGC 5645.[3]

Discoveries

NGC 428 was discovered by William Herschel in December 1786.[2] A type Ia supernova designated SN2013ct was discovered May 11, 2013, within the galaxy by Stuart Parker of the Backyard Observatory Supernova Search (BOSS) project in Australia and New Zealand.[2][4]

Smoker et al. reported in 1996 on the NGC 428 field, with the HI tail and LSB dwarf 0110+008, assessing star formation properties based on molecule density distributions, and concluded that the tail formation most likely originated through tidal interactions between two galaxies.[5]

Further reading

See also

References

  1. 1 2 "Hubble Delivers Gorgeous View of Galaxy 48 Million Light-Years Away". 16 August 2015.
  2. 1 2 3 4 5 "NASA Image of the Day". NGC 428. Retrieved 15 Aug 2015.
  3. NED, No.4. "Notes for object NGC 0428".
  4. "NGC428 discovery".
  5. Smoker, J. V., Davies, R. D., & Axon, D. J. (1996). "H I and optical observations of the NGC 428 field". Monthly Notices of the Royal Astronomical Society 281: 393–405. Bibcode:1996MNRAS.281..393S. doi:10.1093/mnras/281.2.393.

External links

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