Uv Imaging and Spectroscopy of High Excitation Herbig-Haro Objects

Computer Science

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Hst Proposal Id #8042 Interstellar Matter

Scientific paper

Our cycle 7 FUV observations of HH1-2 have identified two knots in HH2 that are bright enough for follow-up spectroscopy. In cycle 8, we will use two of our allotted three orbits to obtain low resolution {G140L} long-slit spectroscopy of these knots in order to identify and map the various ionic and molecular components of the FUV emission. We plan to use the third orbit to obtain low resolution {G750L} long slit spectroscopy of a newly discovered potential HH flow associated with HD-163296 provided that no conflict exists with this new target. If a conflict exists, the remaining orbit will be used for obtaining low resolution spectroscopy of the HH 2 knots.

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