The distribution of Main-Sequence stars in the open cluster NGC 7789

Details The distribution of Main-Sequence stars in the open cluster NGC 7789 The distribution of Main-Sequence stars in the open cluster NGC 7789

Sep 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980ap%26ss..72..233h&link_type=abstract

Astrophysics and Space Science, Volume 72, Issue 1, pp.233-236

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

By star counts on four plates with different limiting magnitudes, it was
found that the relative frequency of Main-Sequence stars increases from
the centre of the cluster to the boundary. It is shown that the stars of
NGC 7789 are separated according to their masses.

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