Hard X-ray spectrum of NGC 4151

Details Hard X-ray spectrum of NGC 4151 Hard X-ray spectrum of NGC 4151

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...221l...7a&link_type=abstract

Astrophysical Journal, Part 2 - Letters to the Editor, vol. 221, Apr. 1, 1978, p. L7-L11.

Astronomy and Astrophysics

Astrophysics

30

Astronomical Spectroscopy, Galactic Radiation, Seyfert Galaxies, X Ray Sources, Ariel 5 Satellite, Balloon-Borne Instruments, Oso-7, Power Spectra, Uhuru Satellite, X Ray Spectra

Scientific paper

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.

Affiliated with

Also associated with

No associations

Rating

Hard X-ray spectrum of NGC 4151 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 Hard X-ray spectrum of NGC 4151, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Hard X-ray spectrum of NGC 4151 will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1379222