The Conference will take place from Monday 8th to Wednesday 10th, September 2014.
The outline of the conference is given below. Early submission of abstracts is welcome
Context
- from IRAS excess to debris disks
- young associations
The beta Pic system
- beta Pic properties
- gaz properties
- dust properties
- planet(s)
- formation and dynamical history
Other debris disks:
- descriptions, similarities/differences with beta Pic (what can the example of beta Pic bring for the study of these objects? what can the example of these objects bring for the study of beta Pic ?)
- BPMG stars
- emblematic systems with IR excess
- disks modeling results
- connection between debris disks and planets
Next decade (beta Pic & other stars with debris disks):
- open questions
- future observations and modeling
