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pro vyhledávání: '"Uliana Sapunova"'
Autor:
Maksim Ozhiganov, Mikhail Medvedev, Varvara Karteyeva, Ruslan Nakibov, Uliana Sapunova, Vadim Krushinsky, Ksenia Stepanova, Anastasia Tryastsina, Aleksandr Gorkovenko, Gleb Fedoseev, Anton Vasyunin
Publikováno v:
The Astrophysical Journal Letters, Vol 972, Iss 1, p L10 (2024)
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 fo
Externí odkaz:
https://doaj.org/article/efbfe524122e4dec8aac84893b9e467e
