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- W4383860405 abstract "Galactic supernova remnants (SNRs) play an important role in our understanding of supernovae and their feedback on the interstellar environment. SNR G352.7$-$0.1 is special for its thermal composite morphology and double-ring structure. We have performed spectroscopic mapping in $^{12}$CO and $^{13}$CO $J=2$-1 lines toward G352.7$-$0.1 with the Atacama Pathfinder Experiment telescope. Broad $^{12}$CO lines are found in the northeastern ring at a local-standard-of-rest velocity range of $sim-50$-$-30$ km s$^{-1}$, suggesting that the remnant is interacting with molecular clouds (MCs) at $sim-51$ km s$^{-1}$. Thus, we adopt a distance of $sim10.5$ kpc for this SNR. The momentum and kinetic energy of the shocked gas along the line of sight are estimated to be $sim10^2{rm M_{sun}}$ km s$^{-1}$ and $sim10^{46}$ erg, respectively. We also find an expanding structure around the remnant, which is possibly related to the wind-blown bubble of the progenitor star. From the Fermi-LAT data in an energy range of 0.1-500 GeV, we find no gamma-ray counterparts of G352.7$-$0.1." @default.
- W4383860405 created "2023-07-11" @default.
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- W4383860405 date "2023-07-06" @default.
- W4383860405 modified "2023-10-16" @default.
- W4383860405 title "Molecular environment of the thermal composite supernova remnant G352.7$-$0.1" @default.
- W4383860405 doi "https://doi.org/10.48550/arxiv.2307.03369" @default.
- W4383860405 hasPublicationYear "2023" @default.
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