2021
DOI: 10.48550/arxiv.2105.08732
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First survey of HCNH$^+$ in high-mass star-forming cloud cores

F. Fontani,
L. Colzi,
E. Redaelli
et al.

Abstract: Context. Most stars in the Galaxy, including the Sun, were born in high-mass star-forming regions. It is hence important to study the chemical processes in these regions to better understand the chemical heritage of both the Solar System and most stellar systems in the Galaxy. Aims. The molecular ion HCNH + is thought to be a crucial species in ion-neutral astrochemical reactions, but so far it has been detected only in a handful of star-forming regions, and hence its chemistry is poorly known. Methods. We hav… Show more

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