Uv Imaging and Spectroscopy of High Excitation Herbig-Haro Objects

Details Uv Imaging and Spectroscopy of High Excitation Herbig-Haro Objects Uv Imaging and Spectroscopy of High Excitation Herbig-Haro Objects

Dec 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997hst..prop.7580k&link_type=abstract

HST Proposal ID #7580

Physics

Hst Proposal Id #7580 Interstellar Matter

Scientific paper

We will use STIS far UV imaging and long-slit spectroscopy to investigate the morphology and physical conditions in high excitation Herbig-Haro objects. FUV imaging in a bandpass containing the CIV emission line will delineate the morphology of high excitation gas and identify regions suitable for followup spectroscopy. Low resolution {G140L} long-slit spectroscopy will identify and map the various ionic and molecular components of the FUV emission. Medium resolution {G140M} long-slit spectroscopy will provide maps of the velocity structure in the CIV emission and will probe the physical conditions producing fluorescent emission from molecular hydrogen.

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