Open-cluster density profiles derived using a kernel estimator

Surface and spatial radial density profiles in open clusters are derived using a kernel estimator method. Formulae are obtained for the contribution of every star into the spatial density profile. The evaluation of spatial density profiles is tested against open-cluster models from N-body experiment...

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Veröffentlicht in:	Monthly notices of the Royal Astronomical Society 2016-03, Vol.456 (4), p.3757-3757
1. Verfasser:	Seleznev, Anton F
Format:	Artikel
Sprache:	eng
Schlagworte:	Astronomy Clusters Comparative analysis Coronas Density Estimators Experiments Kernels Mathematical models Open clusters Stars
Online-Zugang:	Volltext
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