A Yebes W-band Line Survey towards an Unshocked Molecular Cloud of Supernova Remnant 3C 391: Evidence of Cosmic-Ray-Induced Chemistry
Cosmic rays (CRs) have strong influences on the chemistry of dense molecular clouds
(MCs). To study the detailed chemistry induced by CRs, we conducted a Yebes W-band line …
(MCs). To study the detailed chemistry induced by CRs, we conducted a Yebes W-band line …
Mapping the Dense Molecular Gas toward 13 Supernova Remnants
TY Tu, Y Chen, QC Liu - The Astrophysical Journal, 2024 - iopscience.iop.org
Mapping the Dense Molecular Gas toward 13 Supernova Remnants - IOPscience Skip to
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Molecular chemistry induced by J-shock toward supernova remnant W51C
Context. Shock waves from supernova remnants (SNRs) strongly affect the physical and
chemical properties of molecular clouds (MCs). Shocks propagating into magnetized MCs …
chemical properties of molecular clouds (MCs). Shocks propagating into magnetized MCs …
Mapping the dense molecular gas towards thirteen supernova remnants
TY Tu, Y Chen, QC Liu - arXiv preprint arXiv:2411.09138, 2024 - arxiv.org
Supernova remnants (SNRs) can exert strong influence on molecular clouds (MCs) through
interaction by shock wave and cosmic rays. In this paper, we present our mapping …
interaction by shock wave and cosmic rays. In this paper, we present our mapping …