Institut national de recherche scientifique français Univerité Pierre et Marie Curie Université Paris Diderot - Paris 7

Predicted signatures of planet formation and orbital evolution in the emission of protoplanetary discs

lundi 6 décembre 2021, par Clément Baruteau (IRAP, Toulouse)

Lundi 13 dĂ©cembre 2021 à 16h00 , Lieu : En visioconfĂ©rence

The classical picture of protoplanetary discs being smooth, continuous structures of gas and dust has been challenged by the growing number of spatially resolved observations. These observations tell us that rings, gaps, large-scale asymmetries like spirals or arcs are common features of the emission of protoplanetary discs, which are often interpreted as signatures of the presence of unseen planets. During this online seminar, I will present some of our recent work on how the formation and orbital evolution of planets can impact the dynamics and the emission of gas and dust in protoplanetary discs. In particular, I will discuss the possibility that a single giant planet may acquire a substantial eccentricity in its protoplanetary disc, and what observational signatures this mechanism predicts.

Pour assister au séminaire

Avec CarbonFreeConf (qui vous donne accès Ă  plus de fonctionnalitĂ©s, e.g. sondages) :

Avec Zoom :