A possible relation between spectral index and z-distribution for supernova remnants

Details A possible relation between spectral index and z-distribution for supernova remnants A possible relation between spectral index and z-distribution for supernova remnants

Jan 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975a%26a....38..149b&link_type=abstract

Astronomy and Astrophysics, vol. 38, no. 1, Jan. 1975, p. 149-152.

Astronomy and Astrophysics

Astrophysics

4

Galactic Radio Waves, Pulsars, Radio Spectra, Supernova Remnants, B Stars, Crab Nebula, O Stars, Spatial Distribution, Spectral Correlation

Scientific paper

A statistical relation has been found between spectral index and the mean distance from the galactic plane for supernova remnants. Using z-distances calculated from the Sigma-D relationship and the observed spectral indices at radio frequencies for 93 galactic supernova remnants, the mean z-distance is found to vary from 175 pc to 60 pc for remnants with flat and steep spectra, respectively. A possible correlation between flat-spectra supernova remnants and pulsars is discussed.

Affiliated with

Also associated with

No associations

Rating

A possible relation between spectral index and z-distribution for supernova remnants 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 A possible relation between spectral index and z-distribution for supernova remnants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A possible relation between spectral index and z-distribution for supernova remnants will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1749257