The open star clusters M36, M38, NGC 2477

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Astrometry, Astronomical Photography, Open Clusters, Radii, Schmidt Telescopes, Star Distribution, Stellar Mass

Scientific paper

The open star clusters M36, M38 and NGC 2477 were investigated by the strip method on charts of photographs taken with the Schmidt-Spiegel telescope of the German Observatory Hoher List for the first two clusters, and with the Curtis-Schmidt telescope of the Cerro Tololo Interamerican Observatory for the last cluster. Results showed solar masses of 830, 2350 and 4400 respectively as well as radii, and central density measurements.

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