Infrared Spectra of Solid HCN Embedded in Various Molecular Environments for Comparison with the Data Obtained with JWST

Hydrogen cyanide (HCN) molecules serve as an important tracer for the chemical evolution of elemental nitrogen in the regions of star and planet formation. This is largely explained by the fact that N atoms and N _2 molecules are poorly accessible for observation in the radio and infrared (IR) range...

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Bibliographic Details

Published in:	The Astrophysical Journal Letters
Main Authors:	Maksim Ozhiganov, Mikhail Medvedev, Varvara Karteyeva, Ruslan Nakibov, Uliana Sapunova, Vadim Krushinsky, Ksenia Stepanova, Anastasia Tryastsina, Aleksandr Gorkovenko, Gleb Fedoseev, Anton Vasyunin
Format:	Article
Language:	English
Published:	IOP Publishing 2024-01-01
Subjects:	Laboratory astrophysics Ice spectroscopy Interstellar clouds Astrochemistry Interstellar molecules Star forming regions
Online Access:	https://doi.org/10.3847/2041-8213/ad6d5c