Globular Cluster Core Structure and Dynamics (fos 36) -- Cycle 0

Details Globular Cluster Core Structure and Dynamics (fos 36) -- Cycle 0 Globular Cluster Core Structure and Dynamics (fos 36) -- Cycle 0

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990hst..prop.1052b&link_type=abstract

HST Proposal ID #1052

Physics

Hst Proposal Id #1052

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.

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