Globular Cluster Core Structure and Dynamics (fos 36) - Cycle 4 Carryover

Details Globular Cluster Core Structure and Dynamics (fos 36) - Cycle 4 Carryover Globular Cluster Core Structure and Dynamics (fos 36) - Cycle 4 Carryover

Jul 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994hst..prop.5696b&link_type=abstract

HST Proposal ID #5696

Physics

Hst Proposal Id #5696 Stellar Populations

Scientific paper

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

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