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NGC 1901

From Wikipedia, the free encyclopedia
Open cluster in the constellation Dorado
NGC 1901

The open cluster NGC 1901
Observation data
Epoch J2000      Equinox J2000
ConstellationDorado
Right ascension05h 18m 11.0s[1][2]
Declination−68° 27′ 00″[1][2]
Characteristics
Astrometry
Radial velocity (Rv)-1.354 km/s
Distance1,354 ly
(415[3] pc)
Details
Age0.6[4] Gyr
Other designations
ESO 56-SC91, OCL 791

NGC 1901 is anopen cluster in theDoradoConstellation. It has a bright middle and is a little rich, with stars from 7th magnitude downwards. The celestial object was discovered on 30 December 1836 by theBritishastronomerJohn Herschel.[5] The cluster is sparsely populated withGAIA data suggesting a membership of around 80 stars.[6] It is considered unlikely it will survive its next pass through theMilky Way’s galactic plane in about 18 million years time.[6]

References

[edit]
  1. ^ab"NGC 1901". Simbad.
  2. ^ab"NED results for object NGC 1901". NASA/IPAC Extragalactic Database. Retrieved24 July 2016.
  3. ^"WEBDA page for open cluster NGC 1901". WEBDA. Retrieved24 July 2016.
  4. ^Pavani, D. B.; Bica, E.; Dutra, C. M.; Dottori, H.; Santiago, B. X.; Carranza, G.; Díaz, R. J. (August 2001). "Open clusters or their remnants: B and V photometry of NGC 1901 and NGC 1252".Astronomy & Astrophysics.374 (2):554–563.arXiv:astro-ph/0106026.Bibcode:2001A&A...374..554P.doi:10.1051/0004-6361:20010741.ISSN 0004-6361.S2CID 119447371.
  5. ^"NGC 1901". Retrieved24 July 2016.
  6. ^abKos, Janez; de Silva, Gayandhi; Buder, Sven; Bland-Hawthorn, Joss; Sharma, Sanjib; Asplund, Martin; D’Orazi, Valentina; Duong, Ly; Freeman, Ken (2018-08-13)."The GALAH survey and Gaia DR2: (non-)existence of five sparse high-latitude open clusters".Monthly Notices of the Royal Astronomical Society.480 (4):5242–5259.arXiv:1807.00822.Bibcode:2018MNRAS.480.5242K.doi:10.1093/mnras/sty2171.ISSN 0035-8711.
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