Zeta OPH Interstellar Molecules - Cycle 2

Details Zeta OPH Interstellar Molecules - Cycle 2 Zeta OPH Interstellar Molecules - Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.1189e&link_type=abstract

HST Proposal ID #1189

Computer Science

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Hst Proposal Id #1189

Scientific paper

Zeta Oph is one of the best studied lines of sight for interstellar absorption lines. Interstellar observations represent one of the primary scientific objectives of the Goddard High Resolution Spectrograph. The goal of this program is to observe weak absorption lines of interstellar molecules with the highest possible spectral resolution, S/N ratio, photometric precision and wavelength accuracy. These observations will demonstrate the limits of GHRS performance for measurements of very weak spectral features. submitted March 1992 for revised cycle 2 without side 1 use augmentation time if available, baseline time if not Potential augmentation time is 5.0 hours.

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