Imaging of Kepler's supernova remnant

Details Imaging of Kepler's supernova remnant Imaging of Kepler's supernova remnant

Feb 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991pasp..103..194v&link_type=abstract

Astronomical Society of the Pacific, Publications (ISSN 0004-6280), vol. 103, Feb. 1991, p. 194-197. Research supported by NSERC

Astronomy and Astrophysics

Astronomy

4

Imagery, Supernova Remnants, Astronomical Photometry, Emission Spectra, Telescopes

Scientific paper

It is shown that the effects of crowding on images of Kepler's supernova remnant, that were obtained with the 3.6-m CFHT, can be greatly reduced by digitally subtracting a scaled continuum image from a narrow-band H-alpha + forbidden N II image. Attention is drawn to a narrow emission filament that extends for 27 arcsec along the western edge of the optical remnant.

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