Multiplicity, warps and infall: How disturbances drive disc evolution

Add to your list(s) Download to your calendar using vCal

• Daniel Price (Monash University)
• Monday 10 November 2025, 16:00-17:00
• MR14 DAMTP and online.

If you have a question about this talk, please contact Loren E. Held.

A clear takeaway from recent observations of protostellar discs is that a large fraction of them show signs of environmental interaction, in the form of large scale spiral arms, infalling streamers or compact dust discs. I will discuss our attempts to explain various aspects of disc morphology from simple theoretical models and what I think it is telling us about the overall picture of how protostellar discs evolve. I will also reflect on the 50-year-old question on the source of “viscosity” in protostellar discs.

This talk is part of the DAMTP Astrophysics Seminars series.

This talk is included in these lists:

• All CMS events
• CMS Events
• Cambridge Astronomy Talks
• Cosmology, Astrophysics and General Relativity
• DAMTP Astrophysics Seminars
• DAMTP info aggregator
• Interested Talks
• MR14 DAMTP and online
• bld31

Note that ex-directory lists are not shown.