Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV

Details Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV

Oct 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983mnras.205..285a&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 205, Oct. 1983, p. 285-295. Research supported by the S

Astronomy and Astrophysics

Astronomy

18

Astronomical Spectroscopy, Crab Nebula, Gamma Ray Astronomy, Continuous Spectra, Energy Spectra, Gamma Ray Telescopes, Line Spectra

Scientific paper

Results are presented of an experiment to search for γ-ray lines from the Crab Nebula region in the energy range 50 - 2000 keV using a cooled intrinsic germanium detector in a sodium iodide anti-coincidence shield. Some evidence for line features is observed at 404.4 and 1049.6 keV with intensities at the top of the atmosphere of (7.2±2.1)×10-3 and (1.9±0.4)×10-2 photons cm-2 s-1 respectively. A line at 78.9 keV has also been detected which shows some variability with time.

Affiliated with

Also associated with

No associations

Rating

Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV 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 Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gamma-ray line features from the Crab Nebula in the energy range 50-2000 keV will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1194527