Revealing the dust grain size in the inner envelope of the Class i protostar Per-emb-50
Carolina Agurto-Gangas(Max Planck Institute for Extraterrestrial Physics), Tyler L. Bourke(University of Manchester), J. E. Pineda(Max Planck Institute for Extraterrestrial Physics), Michael M. Dunham(Middlebury College), L. Testi(Istituto Nazionale per la Fisica della Materia), Ian Stephens(Center for Astrophysics Harvard & Smithsonian), László Szücs(National Radio Astronomy Observatory), Marco Tazzari(University of Cambridge), P. Caselli(Max Planck Institute for Extraterrestrial Physics), A. Miotello
Cited by 25
Related Papers
Advancing Astrophysics with the Square Kilometre Array
|Unknown|2015|836
From Molecular Cores to Planet‐forming Disks: An<i>SIRTF</i>Legacy Program
|Publications of the Astronomical Society of the Pacific|2003|546
Advancing Astrophysics with the Square Kilometre Array (AASKA14)
|Unknown|2015|513
The ALMA Protostellar Interferometric Line Survey (PILS)
|Astronomy and Astrophysics|2016|401
Variations in the Galactic star formation rate and density thresholds for star formation
|Monthly Notices of the Royal Astronomical Society|2012|352