Search for Interstellar Molecules in Spectra of Three B Stars -- Cycles 1,2,3

Details Search for Interstellar Molecules in Spectra of Three B Stars -- Cycles 1,2,3 Search for Interstellar Molecules in Spectra of Three B Stars -- Cycles 1,2,3

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991hst..prop.1200s&link_type=abstract

HST Proposal ID #1200

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Hst Proposal Id #1200

Scientific paper

The scientfic goal of this program is to check current theoretical understanding of gas phase chemistry in diffuse interstellar clouds and to modify this understanding if necessary. A further goal is to look for evidence of molecule formation other than H2 on interstellar grain surfaces. Signatures of many of the most important molecular species are found in the vaccuum and middle ultraviolet accessible to the HRS. It is proposed to observe HD32656 throughout the HRS wavelength range and HD29647 at a few caroussel settings in the 2.4x104 resolving power mode. These stars are associated with the Taurus Cloud complex. It is also proposed to observe omicron persei in the 105 revolving power mode and combine the new results with those found by observations with the "Copernicus" satellite.

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