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词条 NGC 428
释义

  1. Discoveries

  2. Further reading

  3. See also

  4. References

  5. External links

{{Expand German|NGC 428|date=August 2015}}{{Expand Dutch|NGC 428|date=August 2015}}{{Infobox Galaxy
| name = NGC 428
| image = A mess of stars.jpg
| image_size = 300px
| caption = Hubble image of NGC 428.
| epoch = J2000.0
| constellation name = Cetus[1]
| ra = 01h 12m 55,78s [2]
| dec = + 00 ° 58 '51.6 [2]
| z =
| dist_ly = 48 mly [2]
| type =
| appmag_v = +11.3 [2]
| size_v =
| notes =
| names = NGC 428 • UGC 763 • PGC 4367 • Z 385.28 • MCG + 00-04-36 • IRAS 01103 + 0043 • 2MASX J01125570 + 0058536 • GC 238 • H 2.622 • HIPASS J0112 + 00[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 and lacks well defined arms — 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

  • [https://arxiv.org/abs/1504.06282 H-alpha kinematics of S4G spiral galaxies-II. Data description and non-circular motions]
  • [https://arxiv.org/abs/1505.01497 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

  • Galaxy merger
  • List of galaxies

References

[6]
1. ^{{cite web|url=http://news.softpedia.com/news/hubble-delivers-gorgeous-view-of-galaxy-48-million-light-years-away-489360.shtml|title=Hubble Delivers Gorgeous View of Galaxy 48 Million Light-Years Away|date=16 August 2015}}
2. ^{{cite web | title = NASA Image of the Day | work = NGC 428 | url = http://www.nasa.gov/image-feature/goddard/hubble-sees-a-a-mess-of-stars | accessdate = 15 Aug 2015}}
3. ^{{cite web|url=http://ned.ipac.caltech.edu/cgi-bin/datasearch?search_type=Note_id&objid=56159&objname=NGC%200428&img_stamp=YES&hconst=73.0&omegam=0.27&omegav=0.73&corr_z=1&of=table|author=NED|number=4|title=Notes for object NGC 0428}}
4. ^{{cite web|url=https://www.flickr.com/photos/snimages/8727727968/|title=NGC428 discovery}}
5. ^{{cite journal|title=H I and optical observations of the NGC 428 field|date=1996|author=Smoker, J. V.|author2=Davies, R. D.|author3=Axon, D. J.|last-author-amp=yes|journal=Monthly Notices of the Royal Astronomical Society|bibcode=1996MNRAS.281..393S|doi=10.1093/mnras/281.2.393|volume=281|issue=2|pages=393–405}}
6. ^{{cite simbad|title=NGC 428|date=16 July 2016}}

External links

  • [https://in-the-sky.org/data/object.php?id=420 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
{{Ngc5}}{{galaxy}}

2 : Galaxies discovered in 1786|NGC objects

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