Two open clusters: Twins with different histories

Astronomy and Astrophysics – Astronomy

Scientific paper

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Open Clusters, Stellar Evolution, Stellar Dynamics

Scientific paper

Recent accurate wide-field photometry and radial-velocity studies of the open clusters NGC 3680 and IC 4651 show them to be of identical age ( 1.5 Gyr) and metallicity. Their present spatial structure and mass functions show that they have, nevertheless, undergone very different degrees of dynamical evolution: while IC 4651 shows a fully populated main sequence to at least six magnitudes below the turnoff and only weak signs of mass segregation, NGC 3680 is essentially just a surviving cold core of stars in a very narrow mass range, the initial cluster being perhaps a hundred times more massive than now. These twin clusters thus highlight the importance of environmental factors upon the evolution of the stellar population of open clusters.

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