Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientific paper
2011-10-31
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Contribution to 32nd ICRC, Beijing 11-18 August 2011; 4 pages, 5 figures
Scientific paper
The Cygnus region hosts the most conspicuous star-forming region close to the Sun, embedded in a giant complex of molecular clouds in the Local Arm. We present an analysis of the Fermi-LAT observations of Cygnus intended to probe the cosmic-ray and interstellar-matter content of the region. From gamma-ray data we estimate a total of (8 +5 -1) x 10^6 solar masses of interstellar gas in the complex at a distance of 1.4 kpc. The gamma-ray emission from the atomic gas supports the average HI spin temperature derived from radio absorption/emission pairs to estimate its column densities. The X(CO)=N(H2)/W(CO) ratio derived in the massive Cygnus complex is consistent with other LAT estimates for clouds in the Local and Perseus arms. The mass of dark gas, escaping HI and CO observations but traced by dust and gamma rays, amounts to ~10% of the total. We find an average gamma-ray emissivity per interstellar H atom in the 0.1--100 GeV energy band in good agreement with measurements in other segments of the Local Arm. We infer that the cosmic-ray population averaged over a few hundred parsecs is fairly uniform in density and spectrum along the Local Arm. Despite the presence of potential accelerators and much larger interstellar densities in Cygnus compared to the solar neighborhood, their cosmic-ray populations are similar on such a scale.
Fermi/LAT collaboration for the
Grenier Isabelle A.
Tibaldo Luigi
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