ESOP, a New Fabry-Perot Spectrophotometer. Observations of the Iron Coronal Lines in Puppis A

Details ESOP, a New Fabry-Perot Spectrophotometer. Observations of the Iron Coronal Lines in Puppis A ESOP, a New Fabry-Perot Spectrophotometer. Observations of the Iron Coronal Lines in Puppis A

Sep 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995exa.....6..257d&link_type=abstract

Experimental Astronomy, Volume 6, Issue 3, pp.257-273

Astronomy and Astrophysics

Astronomy

3

Spectrophotometry, Coronal Lines, Fabry-Perot, Supernova Remnant

Scientific paper

In this paper we present a new spectrophotometer ESOP (Expérience Spectroscopique d'Observation des Plasmas). We describe its general features and characteristics. We report the first spectrophotometric results on the Puppis A supernova remnant on the coronal iron line emission. These [FeXIV] observations were in the vicinity of the “Eastern X-ray knot.” We have observed at 30″ scale. In appendices we describe in more details some specific technical points.

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