Hot cores in supernova remnant RX J1713.7-3946 exhibit column density ratios of complex organics, deuterated species, and S/N-bearing molecules that are indistinguishable from those in typical star-forming environments.
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Water binding energy on silicate grains is twice that on ice, enabling local retention and inheritance for terrestrial planets without outer Solar System delivery.
Thermo-chemical models predict that NH3 is undetectable with JWST-MIRI even at high N/H while NO may be detectable, and observations confirm no NH3 detections with one tentative NO in V1094 Sco.
citing papers explorer
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Survival of Molecular Complexity under Recent Supernova Feedback: Detection of Hot Cores in RX J1713.7-3946
Hot cores in supernova remnant RX J1713.7-3946 exhibit column density ratios of complex organics, deuterated species, and S/N-bearing molecules that are indistinguishable from those in typical star-forming environments.
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Astrochemical Inheritance of Terrestrial Planets Water from Local Wet Silicates
Water binding energy on silicate grains is twice that on ice, enabling local retention and inheritance for terrestrial planets without outer Solar System delivery.
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Detecting nitrogen-carriers in the inner regions of protoplanetary disks
Thermo-chemical models predict that NH3 is undetectable with JWST-MIRI even at high N/H while NO may be detectable, and observations confirm no NH3 detections with one tentative NO in V1094 Sco.