Clusters IC 4665 and Cr 359 and a Probable Birthplace of the Pulsar PSR B 1929 + 10

Abstract

–Based on the epicyclic approximation, we have simulated the motion of the young open star clusters IC 4665 and Collinder 359. The separation between the cluster centers is shown to have been minimal 7 Myr ago, 36 pc. We have established a close evolutionary connection between IC 4665 and the Scorpius-Centaurus association — the separation between the… (More)

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Cite this paper

@inproceedings{Bobylev2008ClustersI4, title={Clusters IC 4665 and Cr 359 and a Probable Birthplace of the Pulsar PSR B 1929 + 10}, author={Vadim V. Bobylev}, year={2008} }