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Matches in SemOpenAlex for { <https://semopenalex.org/work/W1990483649> ?p ?o ?g. }

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• W1990483649 startingPage "L61" @default.
• W1990483649 abstract "Supernova remnants (⁠|$=$| SNR) are suggested to be sites of cosmic-ray acceleration. In particular, it has been an issue of keen interest whether cosmic ray protons are being accelerated in a SNR which emits TeV |$gamma$|-rays. A crucial observational test for this is to find dense molecular gas towards the SNR, because such molecular gas can best verify the existence of cosmic-ray protons via pion decay to |$gamma$|-rays. Here, we show that new high-resolution mm-wave observations of interstellar CO molecule have revealed molecular gas at 1 kpc distance interacting with the TeV |$gamma$|-ray SNR G 347.3|$-$|0.5, and that a molecular cloud of |$sim 200$| solar masses is clearly associated with the TeV |$gamma$|-ray peak, providing strong evidence for proton acceleration. We have estimated the total energy of accelerated protons to be |$sim 1048 ,mathrm{erg}$|⁠, which corresponds to an acceleration efficiency of |$sim 0.001$|⁠, posing an observational constraint on the proton acceleration." @default.
• W1990483649 created "2016-06-24" @default.
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• W1990483649 date "2003-10-25" @default.
• W1990483649 modified "2023-10-12" @default.
• W1990483649 title "Discovery of Interacting Molecular Gas toward the TeV Gamma-Ray Peak of the SNR G 347.3–0.5" @default.
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• W1990483649 doi "https://doi.org/10.1093/pasj/55.5.l61" @default.
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