X-ray fluxes of radio-selected remnants

Details X-ray fluxes of radio-selected remnants X-ray fluxes of radio-selected remnants

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001aipc..565..449m&link_type=abstract

YOUNG SUPERNOVA REMNANTS: Eleventh Astrophysics Conference. AIP Conference Proceedings, Volume 565, pp. 449-452 (2001).

Astronomy and Astrophysics

Astrophysics

Supernova Remnants, Radio Sources, X-Ray Sources, X-Ray Bursts

Scientific paper

We report the initial measurements of X-ray fluxes from the RASS for SNRs from the Green catalog. There is a significant correlation between radio and X-ray fluxes, but with approximately two orders of magnitude scatter in X-ray flux at a given radio flux level. Surprisingly, there is no apparent difference in the distributions for shell and for non-shell remnants. Some of the correlation is due to the largest sources being the strongest. Work continues on these measurements, with a goal of obtaining X-ray fluxes or limits on all Green Catalog sources with diameters less than 30 arcminutes. .

Affiliated with

Also associated with

No associations

Rating

X-ray fluxes of radio-selected 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 X-ray fluxes of radio-selected remnants, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray fluxes of radio-selected remnants will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1279801