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Planet forming disks, debris disks and the Solar System

Published online by Cambridge University Press:  12 October 2020

Inga Kamp Open the ORCID record for Inga Kamp [Opens in a new window]
Inga Kamp*
Affiliation:
Kapteyn Astronomical Institute, University of Groningen, Groningen, the Netherlands email: kamp@astro.rug.nl
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Abstract

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VLT instruments and ALMA with their high spatial resolution have revolutionized in the past five years our view and understanding of how disks turn into planetary systems. This talk will briefly outline our current understanding of the physical processes occurring and chemical composition evolving as these disks turn into debris disks and eventually planetary systems like our own solar system. I will especially focus on the synergy between disk structure/evolution modeling and astrochemical laboratory/theoretical work to highlight the most recent advances, and open questions such as (1) how much of the chemical composition in disks is inherited from molecular clouds, (2) the relevance of snowlines for planet formation, and (3) what is the origin of the gas in debris disks and what can we learn from it. For each of the three, I will outline briefly how the combination of theory/lab astrochemistry, astrophysical models and observations are required to advance our understanding.

Keywords

astrochemistryplanetary systems: protoplanetary diskscomets: generalcircumstellar matter
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 15 , Symposium S350: Laboratory Astrophysics: From Observations to Interpretation , April 2019 , pp. 207 - 215
Copyright
© International Astronomical Union 2020

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