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NGC 428
Galaxy in the constellation Cetus From Wikipedia, the free encyclopedia
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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.[3] There appears to be a substantial amount of star formation occurring within NGC 428 and it lacks well defined arms — a telltale sign of a galaxy merger.[3] 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.[4]
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Discoveries

NGC 428 was discovered by William Herschel in December 1786.[3] 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.[3][5]
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.[6]
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Further reading
- H-alpha kinematics of S4G spiral galaxies-II. Data description and non-circular motions
- Comparative internal kinematics of the HII regions in interacting and isolated galaxies: implications for massive star formation modes
- A classical morphological analysis of galaxies in the spitzer survey of stellar structure in galaxies (S4G)
- Kinematics of disk galaxies with known masses of their supermassive black holes. Observations Cherepashchuk, A.; Afanas’ev, V.; Zasov, A.; and Katkov, I. Astronomy Reports, 2010, Vol.54(7), pp. 578–589.
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See also
References
External links
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