pith. machine review for the scientific record. sign in

arxiv: 1203.6271 · v1 · submitted 2012-03-28 · 🌌 astro-ph.IM · astro-ph.EP· astro-ph.SR

Recognition: unknown

Circumstellar disks and planets. Science cases for next-generation optical/infrared long-baseline interferometers

Authors on Pith no claims yet
classification 🌌 astro-ph.IM astro-ph.EPastro-ph.SR
keywords circumstellardisksinfraredinterferometerslong-baselineplanetsevolutionformation
0
0 comments X
read the original abstract

We present a review of the interplay between the evolution of circumstellar disks and the formation of planets, both from the perspective of theoretical models and dedicated observations. Based on this, we identify and discuss fundamental questions concerning the formation and evolution of circumstellar disks and planets which can be addressed in the near future with optical and infrared long-baseline interferometers. Furthermore, the importance of complementary observations with long-baseline (sub)millimeter interferometers and high-sensitivity infrared observatories is outlined.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.