High Resolution STIS Observations of HD 202347

Details High Resolution STIS Observations of HD 202347 High Resolution STIS Observations of HD 202347

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999hst..prop.8402m&link_type=abstract

HST Proposal ID #8402

Computer Science

Hst Proposal Id #8402

Scientific paper

We will observe HD 202347 with STIS at high resolution to determine the velocity structure and abundances of the interstellar gas along the sight line. The object lies in the direction of the Perseus spiral arm, and multiple components are visible in high resolution Ca II data. This object is a likely FUSE ERO object, and as such, the higher resolution STIS data are critical for modeling the velocity structure of the absorption profiles.

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