Globular Cluster Core Structure and Dynamics (fos 36) - Part 2

Details Globular Cluster Core Structure and Dynamics (fos 36) - Part 2 Globular Cluster Core Structure and Dynamics (fos 36) - Part 2

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.6892b&link_type=abstract

HST Proposal ID #6892

Physics

Hst Proposal Id #6892 Stellar Populations

Scientific paper

Obtain data on the stellar populations in the central cores of globularclusters. Clusters with and without central unresolved cusps, and with andwithout central X-ray sources will be observed. Spectra will be obtained atthe center of the UV brightness, and at a distance within about one coreradius. We might expect these spectra to differ; massive objects formed incollisions may produce unexpected spectral features, as well as relativelyintense UV radiation in the central core. WFPC2 imaging data for NGC 1851to be shared with GO program 6095 (Djorgovski et al.)

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