HRI Observations of Balmer Dominated Filaments in the SNR RCW86

Details HRI Observations of Balmer Dominated Filaments in the SNR RCW86 HRI Observations of Balmer Dominated Filaments in the SNR RCW86

Sep 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999stin...9901874l&link_type=abstract

Technical Report, Space Telescope Science Inst. Baltimore, MD United States

Physics

Balmer Series, Visual Observation, Radio Observation, Solar Prominences, X Rays, High Resolution, Spectroscopy, Rosat Mission, Imaging Techniques

Scientific paper

The objective of this project was to use the ROSAT HRI to study the recently discovered optical Balmer-dominated filaments in the young SNR R-CW86. The observations provide complete high-resolution X-ray coverage of the shell of the SNR. These X-ray observations are combined with new optical observations (both imaging and spectroscopic), and new high resolution radio observations to provide a better overall understanding of the state of the remnant (Sedov or reverse shock), its history (as the possible SNR of SN 185 AD), and the physics of non-radiative shocks.

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