Astrophysical parameters of ten poorly studied open star clusters

Details Astrophysical parameters of ten poorly studied open star clusters Astrophysical parameters of ten poorly studied open star clusters

2011-05-13

arxiv.org/abs/1105.2683v2

Astronomy and Astrophysics

Astrophysics

Galaxy Astrophysics

10 pages, 5 figures, 2 tables; accepted in "Research in Astronomy and Astrophysics Journal"

Scientific paper

We present here the fundamental parameters of ten open star clusters, nominated from Kronberger et al. (2006) who presented some new discovered stellar groups on the basis of 2MASS photometry and DSS visual images. Star counts and photometric parameters (radius, membership, distances, color excess, age, luminosity function, mass function, total mass, and the dynamical relaxation time) have been determined for these ten clusters for the first time. In order to calibrate our procedures, the main parameters (distance, age, and color excesses) have been re-estimated for another five clusters, which are studied by Kronberger et al. (2006) as well.

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