A Study of a Small Cluster Candidate in Norma

Details A Study of a Small Cluster Candidate in Norma A Study of a Small Cluster Candidate in Norma

Apr 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981a%26as...44..127j&link_type=abstract

Astronomy and Astrophysics Supplement, Vol. 44, P. 127, 1981

Astronomy and Astrophysics

Astrophysics

Scientific paper

Five stars in the area of the Lodén cluster candidate n°2326 (in Norma) have been photoelectrically observed in UBV and classified on objective prism spectral plates. These observations have been used to calculate the distance to and the colour excess of the cluster candidate. Resulting values are V-MV = 11m.16 ± 0m.94 (s.d.) and EB-V = 0m.41 ± 0m.12 (s.d.) leading to a distance of 0.9 kpc. The earliest spectral type on the main sequence is B9, corresponding to an age of 2x105 years.

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