Early Planet Formation in Embedded Disks (eDisk). II. Limited Dust Settling and Prominent Snow Surfaces in the Edge-on Class I Disk IRAS 04302+2247

Publication: The Astrophysical Journal, Volume 951, Issue 1, id.9, 26 pp.

Summary

While dust disks around optically visible, Class II protostars are found to be vertically thin, when and how dust settles to the midplane are unclear. As part of the Atacama Large Millimeter/submillimeter Array large program, Early Planet Formation in Embedded Disks, we analyze the edge-on, embedded, Class I protostar IRAS 04302+2247, also nicknamed the "Butterfly Star. The results suggest that the dust of this Class I source has yet to vertically settle significantly.
Travis J. Thieme
Travis J. Thieme
Postdoctoral Research Fellow