Hard X-ray spectrum of NGC 4151.
Abstract
The X-ray source 4U 1206+39 associated with the Seyfert galaxy NGC 4151 was observed with the high-pressure proportional chamber of the HXR76 experiment on board the Transatlantic Balloon Facility. The spectrum in the 25-190-keV range may be fitted with a power law with spectral slope alpha = 0.9 + or - 0.2. Data are consistent with previous observations in the same range, and no long-term variability is indicated. Comparison with the low-energy spectrum of Ariel 5 shows a break at about 40 keV where the spectral index becomes harder. Data are also consistent with the Miso gamma experiment in the range 0.15-20 MeV.
- Publication:
-
The Astrophysical Journal
- Pub Date:
- April 1978
- DOI:
- Bibcode:
- 1978ApJ...221L...7A
- Keywords:
-
- Astronomical Spectroscopy;
- Galactic Radiation;
- Seyfert Galaxies;
- X Ray Sources;
- Ariel 5 Satellite;
- Balloon-Borne Instruments;
- Oso-7;
- Power Spectra;
- Uhuru Satellite;
- X Ray Spectra;
- Astrophysics;
- Seyfert Galaxies:X-Ray Sources