Remarks on the Soft X-Ray Emission from the Galactic Radio Spurs

Details Remarks on the Soft X-Ray Emission from the Galactic Radio Spurs Remarks on the Soft X-Ray Emission from the Galactic Radio Spurs

Nov 1972

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1972ap%26ss..19..145r&link_type=abstract

Astrophysics and Space Science, Volume 19, Issue 1, pp.145-149

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

It is pointed out that the all old supernova remnants are not in general sources of soft X-ray emission. Again it is pointed out that the galactic radio spur (Cetus arc) may be an old supernova remnant but it has already ceased to be a source of X-ray emission. Finally X-ray flux from Vela is ostimated from cooling rate of neutron star by neutrino emission. The results agree approximately with the observed X-ray flux from Vela X.

Affiliated with

Also associated with

No associations

Rating

Remarks on the Soft X-Ray Emission from the Galactic Radio Spurs 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 Remarks on the Soft X-Ray Emission from the Galactic Radio Spurs, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Remarks on the Soft X-Ray Emission from the Galactic Radio Spurs will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1867668