University of Cambridge > Talks.cam > DAMTP Astrophysics Seminar > Vorticies from low-mass planet formation in "transition discs”

Vorticies from low-mass planet formation in "transition discs”

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

If you have a question about this talk, please contact Dr William Béthune.

I will describe how so-called “transition discs” are natural sites for the trapping of pebble-sized dust particles. Consequently these pebble traps are natural sites for pebble accretion. I will argue that rapid pebble accretion can lead to the disc becoming locally baroclinic and prone to the formation of anti-cyclonic vorticies. I will then sketch out an evolutionary cycle of vortex formation and destruction and relate this mechanism to the observed asymmetries in “transition discs”.

This talk is part of the DAMTP Astrophysics Seminar series.

Tell a friend about this talk:

This talk is included in these lists:

Note that ex-directory lists are not shown.

 

© 2006-2017 Talks.cam, University of Cambridge. Contact Us | Help and Documentation | Privacy and Publicity