Stellar Formation and Evolution (WF/PC-17) Cycle 1

Details Stellar Formation and Evolution (WF/PC-17) Cycle 1 Stellar Formation and Evolution (WF/PC-17) Cycle 1

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.3188w&link_type=abstract

HST Proposal ID #3188

Physics

Hst Proposal Id #3188

Scientific paper

High resolution images will be obtained for a small number of T Tauri stars, Her big-Haro objects, and objects whose evolutionary state is uncertain. Most of the young stellar objects are in the Taurus complex, which is near enough that the high resolution afforded by ST will explore physical scales never before seen in these objects. Limited temporal coverage will also be obtained to search for structural variations at small scales.

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