Astronomy and Astrophysics – Astronomy
Scientific paper
Jan 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992a%26a...253..145s&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 253, no. 1, Jan. 1992, p. 145-149.
Astronomy and Astrophysics
Astronomy
28
Black Holes (Astronomy), Gamma Ray Astronomy, Stellar Spectra, X Ray Binaries, Energy Spectra, Gamma Ray Telescopes, O Stars, Spaceborne Telescopes, Supergiant Stars
Scientific paper
Image, energy spectra and timing data results are presented from March 23-24, 1990 observations conducted toward Cyg X-1 with the orbiting coded-aperture SIGMA telescope in the 35 keV to 1.3 MeV range. The source has been detected up to about 500 keV with high statistical significance. The best fit of an analytical shape to the derived photon spectrum corresponds to a Comptonized model. Millisec-resolution timing data confirm the variability down to 80-msec timescales previously detected by HEAO-1.
Ballet Jean
Bonazzola Silvano
Chulkov I.
Churazov Eugene
Cordier Bertand
No associations
LandOfFree
Soft gamma ray observations of Cygnus X-1 with the coded-aperture SIGMA telescope 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 Soft gamma ray observations of Cygnus X-1 with the coded-aperture SIGMA telescope, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Soft gamma ray observations of Cygnus X-1 with the coded-aperture SIGMA telescope will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-933449