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astro-ph.SR2020★ 23 cited
Resolved molecular line observations reveal an inherited molecular layer in the young disk around TMC1A
Daniel Harsono, Matthijs van der Wiel, Per Bjerkeli +4
Physical processes that govern the star and planet formation sequence influence the chemical composition and evolution of protoplanetary disks. To understand the chemical compositi…
astro-ph.SR2020
Linking ice and gas in the Serpens low-mass star-forming region
G. Perotti, W. R. M. Rocha, J. K. Jørgensen +3
The interaction between dust, ice, and gas during the formation of stars produces complex organic molecules. While observations indicate that several species are formed on ice-cove…