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- W2753253661 abstract "We searched for the γ-ray signal from M33, one of the largest galaxies in the Local Group, using the Pass8 data from the Fermi Large Area Telescope (LAT). No statistically significant γ-ray emission has been detected in the direction of M33, and we report a new upper limit of the high-energy ( > 100 MeV) photon flux of 2.3 × 10− 9 ph cm− 2 s− 1, which is stricter than previous constraints and implies a cosmic ray density for M33 that is lower than that suggested previously. The current limit is still, however, in agreement with the correlation of star formation rate and γ-ray luminosity inferred from the Local group galaxies and a few nearby starburst galaxies." @default.
- W2753253661 created "2017-09-15" @default.
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- W2753253661 date "2017-08-04" @default.
- W2753253661 modified "2023-10-17" @default.
- W2753253661 title "Search for the γ-ray emission from M33 with the Fermi Large Area Telescope" @default.
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- W2753253661 doi "https://doi.org/10.1093/mnras/stx929" @default.
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