Pc Images of Eta Carinae Core - Cycle 2

Details Pc Images of Eta Carinae Core - Cycle 2 Pc Images of Eta Carinae Core - Cycle 2

Jul 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992hst..prop.3209e&link_type=abstract

HST Proposal ID #3209

Physics

Hst Proposal Id #3209

Scientific paper

This is a new proposal submitted in March, 1992 to define PC exposures of the core of Eta Carinae. The new PC images include explicit exposures of a nearby star for the purpose of deriving a valid PSF. The orientation is specified to allow Eta Carinae itself to remain visible on the PC when the pointing is shifted to position the PSF star on PC6. The images are made in a line free violet continuum and in a line free red continuum F631N (this is a O I line filter, but there is negligible O I emission in the core of Eta Carinae.) This proposal uses GTO baseline time.

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