Mass distribution in the open cluster NGC 1664

Details Mass distribution in the open cluster NGC 1664 Mass distribution in the open cluster NGC 1664

May 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998an....319..187m&link_type=abstract

Astronomische Nachrichten, vol. 319, no. 3, p. 187.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

We start with the hypotheses that the cluster space is limited by an ellipsoid with a semiprincipal axis directed to the observer and that the star density inside of concentric ellipsoidal layers remains constant, although varying from layer to layer. It results that the mean star mass at the periphery of the cluster is 0.59 Sun masses smaller than that at the center.

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