NGC 428
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NGC 428 | |
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![]() Hubble image of NGC 428.
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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
- 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.
See also
References
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External links
- The galaxy NGC 428 (Location dependent info when to observe the galaxy in the sky)
- Supernovae 2013ct in NGC 428
- NASA/IPAC Extragalactic Database
- Images of NGC 428
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