HEAO 1 measurements of the galactic ridge
Abstract
The HEAO A2 experiment data was systematically searched for unresolved galactic disc emission. Although there were suggestions of non-uniformities in the emission, the data were consistent with a disc of half-thickness 241 + 22 pc and surface emissivity (2-10 keV) at galactic radius R(kpc) of 2.2 10 to the minus 7th power exp(-R/3.5) erg/sq cm to the (-2)power/s (R 7.8 kpc). giving a luminosity of approximately 4.4 10 to the 37th power erg S to the (-1) power. If the model is extrapolated to radii less than 7.8 kpc, the unresolved disc emission is approximately 1.4 10 to the 38th power erg S to the (-1) power (2-10 keV) i.e., a few percent of the luminosity of the galaxy in resolved sources. the disc emission has a spectrum which is significantly softer than that of the high galactic latitude diffuse X-ray background and it is most probably of discrete source origin.
- Publication:
-
NASA STI/Recon Technical Report N
- Pub Date:
- October 1981
- Bibcode:
- 1981STIN...8220097W
- Keywords:
-
- Absorption Spectra;
- Astronomical Models;
- Compton Effect;
- Emission Spectra;
- Galactic Radiation;
- Galactic Structure;
- Heao 2;
- X Ray Sources;
- Astrophysics;
- Bremsstrahlung;
- Gamma Rays;
- Hydrogen;
- Intergalactic Media;
- Luminosity;
- Mathematical Models;
- Radiant Flux Density;
- Synchrotron Radiation;
- Astrophysics