X-ray emission from the supernova remnant G287.8-0.5

Details X-ray emission from the supernova remnant G287.8-0.5 X-ray emission from the supernova remnant G287.8-0.5

Jun 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976stin...7627135b&link_type=abstract

Unknown

Astronomy and Astrophysics

Astronomy

Supernova Remnants, X Ray Sources, Oso, Supernovae, X Ray Astronomy, X Ray Spectroscopy

Scientific paper

The GSFC Cosmic X-ray spectroscopy experiment on OSO-8 observed a weak galactic X-ray source near theta 2 at 288 deg, b2 at -1 deg. The spectrum for this source between 2-20 keV is well represented by a thermal spectrum of kT = 7.34(+3.6),-2.6 keV with an intense iron emission line centered at 6.5 + or - .2 keV. The error box of the Uhuru source 4U1043-59, the only known X-ray source in our field of view, contains the radio supernova remnant G287.8-0.5. The possible association of the X-ray source with this supernova remnant is discussed.

Affiliated with

Also associated with

No associations

Rating

X-ray emission from the supernova remnant G287.8-0.5 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 emission from the supernova remnant G287.8-0.5, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray emission from the supernova remnant G287.8-0.5 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1785249