Submillimeter observations of molecular gas interacting with the supernova remnant W28
arXiv:2211.06100 · doi:10.1051/0004-6361/202037564
Abstract
Context: Supernovae (SNe) inject large amounts of energy and chemically enriched materials into their surrounding interstellar medium and, in some instances, into molecular clouds (MCs). The interaction of a supernova remnant (SNR) with a MC plays a crucial role in the evolution of the cloud's physical and chemical properties. Despite their importance, only a handful of studies have been made addressing the molecular richness in MCs impacted by SNRs. (Sub)millimter wavelength observations of SNR-MC can be used to build a census of their molecular richness, which in turn can motivate various chemical and physical models aimed at explaining the chemical evolution of the clouds. Aims: We carried out multi-molecule/multi-transition observations toward the region F abutting the SNR W28. We used the detected lines to constrain the physical conditions of this region. Methods: We used the APEX Telescope to observe molecular lines in the frequency from . We used non-LTE RADEX modeling to interpret the observational data. Results: We detected emission from multiple molecular species, namely CHOH, HCO, SO, SiO, CN, CCH, NO, CS, HCO, HCN, HNC, NH, CO, and from isotopologues of some of them. We report the first detection of thermally excited (non-maser) CHOH emission toward a SNR. Employing non-LTE RADEX modeling of multiple HCO and CHOH lines, we constrain the kinetic temperature from 60 to 100K and the gas density from to . We obtained an ortho-para ratio 2 for HCO, which indicates that formaldehyde is most likely formed on dust grain surfaces. Conclusions: Our results show that molecules as complex as HCO and CHOH can be detected in SNR-MC interactions. This could motivate chemical modelling to explore their formation pathways.
arXiv comment19 pages, 13 figures, 6 tables, accepted to A&A
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