Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1981
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981stin...8122995j&link_type=abstract
Presented at the 2d Reunion Latino-Am. de la Union de Astron. Intern., Merida, Venezuela
Astronomy and Astrophysics
Astronomy
Galactic Radiation, Gamma Ray Astronomy, Gamma Ray Spectra, Milky Way Galaxy, Balloon-Borne Instruments, Flux (Rate), Galactic Structure, Photons, Positron Annihilation, Positrons
Scientific paper
The detection of the 0.511 MeV electron positron annihilation line coming from the Galactic Center to provide the means to estimate the rate of positron production and to test some theoretical sources of positrons is addressed. The results of the measurements of the 0.511 MeV line flux made with a gamma ray experiment on board a stratospheric balloon are presented. The detector field of view looked at the galactic longitude range -31 deg l(II) +41 deg. The observed flux is 0.0067 (+ or - 0.0005) photons 1/cm(2)5 which is in very good agreement with the expected flux when assuming that the Galactic Center is a line source emitting uniformly.
Benson Jennifer L.
Jardim O. D. J.
Jardim V. A. M.
Martin Inácio M.
No associations
LandOfFree
Measurement of the 0.511 MeV gamma ray line from the Galactic Center 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 Measurement of the 0.511 MeV gamma ray line from the Galactic Center, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Measurement of the 0.511 MeV gamma ray line from the Galactic Center will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1409080