Weak Interstellar Lines in the Spectrum of Zeta OPH

Details Weak Interstellar Lines in the Spectrum of Zeta OPH Weak Interstellar Lines in the Spectrum of Zeta OPH

Jul 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995hst..prop.6323e&link_type=abstract

HST Proposal ID #6323

Physics

Hst Proposal Id #6323 Interstellar Medium

Scientific paper

This proposal defines observations of four wavelengths in the interstellar spectrum of Zeta Ophiuchi. All are made with Echelle A, and will achieve signal to noise ratios near 350 per data point. The spectral regions include weak interstellar absorption lines of molecules, heavy elements and high ionization species that have not been detected in GHRS data with lower resolution and signal to noise.

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