Optical observations of the supernova remnant AX J2001+3235

(2) Foundation for Research; E.V. Paleologou (2) ((1) Department of Physics; F. Mavromatakis (1); P. Boumis (1); Technology-Hellas (Greece)); University of Crete (Greece)

arxiv: astro-ph/0111593 · v1 · submitted 2001-11-30 · 🌌 astro-ph

Optical observations of the supernova remnant AX J2001+3235

F. Mavromatakis (1) , P. Boumis (1) , E.V. Paleologou (2) ((1) Department of Physics , University of Crete (Greece) , (2) Foundation for Research , Technology-Hellas (Greece)) This is my paper

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keywords emissionimageshalphaobtainedoiiiopticalanalysiscomplex

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We present results from a first analysis of optical data on G 69.4+2.4 obtained with the 0.3 m and 1.3 m telescopes at Skinakas Observatory. Filamentary emission is detected in the [OIII] 5007 A and Halpha+[NII] images oriented in the south-west, north-east direction. The Halpha+[NII] images reveal a complex network of filaments, while the [OIII] images show a single filament. Low resolution spectra were also obtained which identify the observed emission as emission from shock heated gas.

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Optical observations of the supernova remnant AX J2001+3235

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