no code implementations • 27 Feb 2020 • Daniel Harsono, Magnus Persson, Alyssa Ramos, Nadia Murillo, Luke Maud, Michiel Hogerheijde, Arthur Bosman, Lars Kristensen, Jes Jorgensen, Ted Bergin, Ruud Visser, Joe Mottram, Ewine van Dishoeck
Our observations are sensitive to the emission from the known Keplerian disks around three out of the five Class I objects in the sample.
Solar and Stellar Astrophysics Earth and Planetary Astrophysics Astrophysics of Galaxies
