Study of dust and ices properties in highly inclined protoplanetary disks
Thesis defense of Laurine Martinien - Wednesday, October 7th octobre at 10.00 am - Manuel Forestini room IPAG
Planets form in protoplanetary disks surrounding young stars. Composed of gas, dust, and ices, these disks are the location of grain growth, during which particles coagulate and grow from a few micrometers to bodies several thousand kilometers in size. However, the physical mechanisms driving this growth remain poorly constrained. The study of micrometer- and millimeter-sized dust provides valuable insights into the early stages of planet formation. In addition, ices (H2O, CO2, and CO) have (…)
Read more
The federation
Intranet
