X-ray emission from U Geminorum and the radio spur at L about 200 deg

Details X-ray emission from U Geminorum and the radio spur at L about 200 deg X-ray emission from U Geminorum and the radio spur at L about 200 deg

Feb 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apl....16...67n&link_type=abstract

Astrophysical Letters, vol. 16, no. 2, 1975, p. 67-69.

Astronomy and Astrophysics

Astronomy

3

Astronomical Models, Radio Sources (Astronomy), Stellar Luminosity, X Ray Astronomy, Emission Spectra, Energy Distribution, Rocket-Borne Instruments, Spectrum Analysis

Scientific paper

Rocket X-ray data on U Geminorum obtained at phase 0.062 during a quiescent period are shown to yield an upper limit of 7 times 10 to 31 erg/sec for the X-ray luminosity in the 150 to 280 eV band. This limit is compared with the recent reported X-ray observation of SS Cygni during an active period and the prediction of Warner's model for U Gem. It is suggested, in agreement with Berkhuijsen, that a soft X-ray feature at l about 200 deg and b about +20 deg arises from a radio spur at that location.

Affiliated with

Also associated with

No associations

Rating

X-ray emission from U Geminorum and the radio spur at L about 200 deg 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 U Geminorum and the radio spur at L about 200 deg, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and X-ray emission from U Geminorum and the radio spur at L about 200 deg will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-998912