Imaging and Polarimetry of Yso's

Details Imaging and Polarimetry of Yso's Imaging and Polarimetry of Yso's

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7228y&link_type=abstract

HST Proposal ID #7228

Computer Science

Hst Proposal Id #7228 Young Stars And Circumstellar Material

Scientific paper

The immediate environs of a number of well known Young Stellar Objects will be investigated with coronagraphic imaging, polarimetry, and line imaging. The majority of these objects are associated with molecular outflows, and the line imaging will investigate the interaction between outflow and the surrounding interstellar medium. The lines Paschen-alpha, S{1} molecular hydrogen, and [Fe II] will allow us to sample both the molecular and ionized gas components. The stable and high resolution observing conditions possible with NICMOS will permit very high angular resolution polarimetry. The dust scattering morphology of extended disks can be studied with these observations.

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