Optical identification of supernova remnants in M33

Details Optical identification of supernova remnants in M33 Optical identification of supernova remnants in M33

Feb 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pasp...91...62s&link_type=abstract

Astronomical Society of the Pacific, Publications, vol. 91, Feb.-Mar. 1979, p. 62-64. Research supported by the Consiglio Nazion

Physics

Optics

11

Astronomical Photography, Galactic Radiation, Nebulae, Supernova Remnants, Astronomical Spectroscopy, Cassegrain Optics, H Alpha Line, H Ii Regions, Image Tubes

Scientific paper

This note reports the identification of 11 supernova remnant (SNR) candidates in a field 22 arcmin in diameter centered on M33, excluding the nuclear region. The SNR candidates were distinguished from H II regions on the basis of optical appearance on direct red plates and the presence of strong forbidden S II emission relative to (H-alpha + forbidden N II) emission. Finding charts and essential data on the SNR candidates are provided, and some properties of the individual objects are discussed.

Affiliated with

Also associated with

No associations

Rating

Optical identification of supernova remnants in M33 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Optical identification of supernova remnants in M33, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Optical identification of supernova remnants in M33 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-830752