A statistical study of the correlation of Galactic supernova remnants with spiral arms and the disk is presented. SNR apparently have a larger radial scale length than disk stars. We estimate that only about 10 percent of the Galactic SNR have been detected.
CITATION STYLE
Li, Z., Wheeler, J. C., Bash, F. N., & Jefferys, W. H. (1988). A Statistical Study of the Correlation of Galactic Supernova Remnants and Spiral Arms. International Astronomical Union Colloquium, 101, 485–488. https://doi.org/10.1017/s0252921100102891
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