Deep optical observations and study of the VRO supernova remnant

Details Deep optical observations and study of the VRO supernova remnant Deep optical observations and study of the VRO supernova remnant

Jan 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012hell.conf...27b&link_type=abstract

10th Hellenic Astronomical Conference, Proceedings of the conference held at Ioannina, Greece, 5-8 September 2011. Edited by Io

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We present the first CCD images of the VRO (G 166.0+4.3) supernova remnant in HI+[N II], [O III] 5007 and [S II] at a moderate angular resolution. Low and high-dispersion spectroscopy was also performed at selected areas around this extended remnant. Diagnostic diagrams of the line intensities from the present spectra and the new kinematical observations both confirm the supernova origin. Taking into account our results (i.e. shock velocities, morphological characteristics etc.) together with observations in other wavelengths (i.e. radio), we provide significant information of the interaction between this SNR and the surrounding ISM.

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