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Autor:
Dana E. Anderson, L. Ilsedore Cleeves, Geoffrey A. Blake, Chunhua Qi, Edwin A. Bergin, John M. Carpenter, Kamber R. Schwarz, Claire Thilenius, Ke Zhang
Publikováno v:
The Astrophysical Journal, Vol 966, Iss 1, p 84 (2024)
Molecular emission is used to investigate both the physical and chemical properties of protoplanetary disks. Therefore, to derive disk properties accurately, we need a thorough understanding of the behavior of the molecular probes upon which we rely.
Externí odkaz:
https://doaj.org/article/8a4a54bf8ec54d7280bdb476ea09eb80