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Chemical complexity in feedback from supernova remnants: first detection of PO+ in IC443 and W44

Cosentino, G. et al.
arXiv (All) · Papers
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astrophysics-of-galaxieshigh-energy-astrophysical-phenomenasolar-and-stellar-astrophysics
Supernova remnant (SNR) may shape the physical and chemical properties of star formation. By releasing refractory elements into the gas phase, they inject material of pre-biotic relevance into molecular clouds. Such elements may be inherited by planetary systems and become relevant for the emergence
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