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NGC 1755

From Wikipedia, the free encyclopedia
Open cluster in the constellation Dorado
NGC 1755
NGC 1755 (Hubble)
Observation data (J2000epoch)
Right ascension04h 55m 16.390s[1]
Declination−68° 12′ 23.12″[1]
Distance160,000[2] ly (49,000 pc)
Absolute magnitude (V)9.9[3]
Apparent dimensions (V)2.6′[3]
Physical characteristics
Estimated age80[4] Myr
Other designationsESO 56-SC28
Associations
ConstellationDorado
See also:Open cluster,List of open clusters

NGC 1755 (also known asESO 56-SC28)[3] is anopen star cluster in theLarge Magellanic Cloud in theDorado constellation. It is about 120 light years across and due to its size could be aglobular cluster.[2] It has a diameter of 2.6′ and an apparent magnitude of 9.9.[3] It was discovered byJames Dunlop in 1826.[2]

References

[edit]
  1. ^ab"NGC 1755".SIMBAD.Centre de données astronomiques de Strasbourg. Retrieved13 February 2021.
  2. ^abc"NGC 1755 (= an OCL in the LMC)". cseligman. Retrieved28 July 2015.
  3. ^abcd"Open cluster NGC 1755". dso-browser. Archived fromthe original on 24 October 2017. Retrieved28 July 2016.
  4. ^Milone, A. P.; Marino, A. F.; d'Antona, F.; Bedin, L. R.; Da Costa, G. S.; Jerjen, H.; MacKey, A. D. (2016)."Multiple stellar populations in Magellanic Cloud clusters. IV. The double main sequence of the young cluster NGC 1755".Monthly Notices of the Royal Astronomical Society.458 (4): 4368.arXiv:1603.03493.Bibcode:2016MNRAS.458.4368M.doi:10.1093/mnras/stw608.

External links

[edit]
  • Media related toNGC 1755 at Wikimedia Commons


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