GRIS observations of Al-26 gamma-ray line emission from two points in the Galactic plane

Details GRIS observations of Al-26 gamma-ray line emission from two points in the Galactic plane GRIS observations of Al-26 gamma-ray line emission from two points in the Galactic plane

Jul 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991apj...375l...9t&link_type=abstract

Astrophysical Journal, Part 2 - Letters (ISSN 0004-637X), vol. 375, July 1, 1991, p. L9-L12.

Other

8

Emission Spectra, Galactic Nuclei, Gamma Ray Spectrometers, Line Spectra, Milky Way Galaxy, Balloon Flight, Heao 3, Imaging Spectrometers

Scientific paper

Both of the Gamma-Ray Imaging Spectrometer (GRIS) experiment's two observations of the Galactic center region, at l = zero and 335 deg respectively, detected Al-26 gamma-ray line emission. While these observations are consistent with the assumed high-energy gamma-ray distribution, they are consistent with other distributions as well. The data suggest that the Al-26 emission is distributed over Galactic longitude rather than being confined to a point source. The GRIS data also indicate that the 1809 keV line is broadened.

Affiliated with

Also associated with

No associations

Rating

GRIS observations of Al-26 gamma-ray line emission from two points in the Galactic plane 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 GRIS observations of Al-26 gamma-ray line emission from two points in the Galactic plane, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and GRIS observations of Al-26 gamma-ray line emission from two points in the Galactic plane will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-861341