NGC 428

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NGC 428
A mess of stars.jpg
Hubble image of NGC 428.
Observation data (J2000.0 epoch)
Constellation Cetus[1]
Distance 48 mly [2]
See also: Galaxy, List of galaxies

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

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External links

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