Planet formation with different gas depletion timescales: Comparing with observations

This paper mainly focus on the influence of N-body interaction in the later stage of planets formation, especially the gas depleted timescale. We want to interpret the distribution of eccentricity comparing with observations.

Bibliographic Details
Main Authors: Wang S., Zhou J.-L., Liu H.
Format: Article
Language:English
Published: EDP Sciences 2011-07-01
Series:EPJ Web of Conferences
Online Access:http://dx.doi.org/10.1051/epjconf/20111605004
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spelling doaj-97ba6979e9874714ae57d700fc3041e62021-08-02T01:02:23ZengEDP SciencesEPJ Web of Conferences2100-014X2011-07-01160500410.1051/epjconf/20111605004Planet formation with different gas depletion timescales: Comparing with observationsWang S.Zhou J.-L.Liu H.This paper mainly focus on the influence of N-body interaction in the later stage of planets formation, especially the gas depleted timescale. We want to interpret the distribution of eccentricity comparing with observations. http://dx.doi.org/10.1051/epjconf/20111605004
collection DOAJ
language English
format Article
sources DOAJ
author Wang S.
Zhou J.-L.
Liu H.
spellingShingle Wang S.
Zhou J.-L.
Liu H.
Planet formation with different gas depletion timescales: Comparing with observations
EPJ Web of Conferences
author_facet Wang S.
Zhou J.-L.
Liu H.
author_sort Wang S.
title Planet formation with different gas depletion timescales: Comparing with observations
title_short Planet formation with different gas depletion timescales: Comparing with observations
title_full Planet formation with different gas depletion timescales: Comparing with observations
title_fullStr Planet formation with different gas depletion timescales: Comparing with observations
title_full_unstemmed Planet formation with different gas depletion timescales: Comparing with observations
title_sort planet formation with different gas depletion timescales: comparing with observations
publisher EDP Sciences
series EPJ Web of Conferences
issn 2100-014X
publishDate 2011-07-01
description This paper mainly focus on the influence of N-body interaction in the later stage of planets formation, especially the gas depleted timescale. We want to interpret the distribution of eccentricity comparing with observations.
url http://dx.doi.org/10.1051/epjconf/20111605004
work_keys_str_mv AT wangs planetformationwithdifferentgasdepletiontimescalescomparingwithobservations
AT zhoujl planetformationwithdifferentgasdepletiontimescalescomparingwithobservations
AT liuh planetformationwithdifferentgasdepletiontimescalescomparingwithobservations
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