Gas Kinematics and Cosmic-Ray Acceleration in the Gamma-Ray SNRs W41 and G22.7–0.2
Year: 2026
Type: article
Abstract: We present a study of the interstellar medium associated with the two middle-aged supernova remnants (SNRs) W41 and G22.7–0.2, both detected in TeV gamma rays. Using high-angular-resolution 12 CO( J = 1–0) data from the Nobeyama 45 m telescope and H i data from the Very Large Array, we investigated the spatial and kinematic properties of molecular and atomic gas that interact with the SNRs. We identified associated clouds in the velocity ranges of +50 to +80 km s −1 for W41 and +76 to +110 km s −1 for G22.7–0.2. Column density analysis indicates that target protons are dominated by molecular hydrogen, while atomic hydrogen contributes less than ∼10%–15% even after correction for self-absorption. The mean proton densities are ∼1.2 × 10 3 cm −3 for W41 and ∼5.3 × 10 2 cm −3 for G22.7–0.2. From the gamma-ray luminosities, we estimate the total energy of accelerated cosmic-ray protons as W p ∼ 3 × 10 47 erg for W41 and ∼1 × 10 48 erg for G22.7–0.2, corresponding to 0.03%–0.1% of the canonical supernova explosion energy. These W p values agree with the decreasing trend in W p observed in the middle-aged SNRs within the previously reported SNR age– W p relation.
Source: The Astrophysical Journal
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: gold
Estimated APC paid: $4,499
OpenAlex ID: W7148481985