Non-Radiative Heating in Pre-Main Sequence Stars: Cycle 2 Continuation

Details Non-Radiative Heating in Pre-Main Sequence Stars: Cycle 2 Continuation Non-Radiative Heating in Pre-Main Sequence Stars: Cycle 2 Continuation

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.1209w&link_type=abstract

HST Proposal ID #1209

Physics

Hst Proposal Id #1209

Scientific paper

We shall obtain UV line fluxes and selected line profiles, using the
HRS, for a diverse sample of pre-main sequence stars. We propose to
study the atmospheric heating, dynamics, and density structure of these
stars.

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