Inside-out planet formation. III. Planet-disk interaction at the dead zone inner boundary

Xiao Hu; Zhaohuan Zhu; Jonathan C. Tan; Sourav Chatterjee

doi:10.3847/0004-637X/816/1/19

Inside-out planet formation. III. Planet-disk interaction at the dead zone inner boundary

Xiao Hu, Zhaohuan Zhu, Jonathan C. Tan, Sourav Chatterjee

CIERA - Center for Interdisciplinary Exploration and Research in Astrophysics

Research output: Contribution to journal › Article › peer-review

25 Scopus citations

Abstract

The Kepler mission has discovered more than 4000 exoplanet candidates. Many of them are in systems with tightly packed inner planets. Inside-out planet formation (IOPF) has been proposed as a scenario to explain these systems. It involves sequential in situ planet formation at the local pressure maximum of a retreating dead zone inner boundary (DZIB). Pebbles accumulate at this pressure trap, which builds up a pebble ring.

Original language	English (US)
Article number	19
Journal	Astrophysical Journal
Volume	816
Issue number	1
DOIs	https://doi.org/10.3847/0004-637X/816/1/19
State	Published - Jan 1 2016

Keywords

planetdisk interactions
planets and satellites: formation
protoplanetary disk

ASJC Scopus subject areas

Astronomy and Astrophysics
Space and Planetary Science

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10.3847/0004-637X/816/1/19

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abstract = "The Kepler mission has discovered more than 4000 exoplanet candidates. Many of them are in systems with tightly packed inner planets. Inside-out planet formation (IOPF) has been proposed as a scenario to explain these systems. It involves sequential in situ planet formation at the local pressure maximum of a retreating dead zone inner boundary (DZIB). Pebbles accumulate at this pressure trap, which builds up a pebble ring.",

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AU - Chatterjee, Sourav

PY - 2016/1/1

Y1 - 2016/1/1

N2 - The Kepler mission has discovered more than 4000 exoplanet candidates. Many of them are in systems with tightly packed inner planets. Inside-out planet formation (IOPF) has been proposed as a scenario to explain these systems. It involves sequential in situ planet formation at the local pressure maximum of a retreating dead zone inner boundary (DZIB). Pebbles accumulate at this pressure trap, which builds up a pebble ring.

AB - The Kepler mission has discovered more than 4000 exoplanet candidates. Many of them are in systems with tightly packed inner planets. Inside-out planet formation (IOPF) has been proposed as a scenario to explain these systems. It involves sequential in situ planet formation at the local pressure maximum of a retreating dead zone inner boundary (DZIB). Pebbles accumulate at this pressure trap, which builds up a pebble ring.

KW - planetdisk interactions

KW - planets and satellites: formation

KW - protoplanetary disk

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M1 - 19

ER -

Inside-out planet formation. III. Planet-disk interaction at the dead zone inner boundary

Abstract

Keywords

ASJC Scopus subject areas

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