Terrestrial planet formation in low-mass disks: dependence with initial conditions

Content Provider	Scilit
Author	Ronco, M. P. de Elía, G. C. Guilera, O. M.
Copyright Year	2014
Description	In general, most of the studies of terrestrial-type planet formation typically use ad hoc initial conditions. In this work we improved the initial conditions described in Ronco & de Elía (2014) starting with a semi-analytical model wich simulates the evolution of the protoplanetary disk during the gas phase. The results of the semi-analytical model are then used as initial conditions for the N-body simulations. We show that the planetary systems considered are not sensitive to the particular initial distribution of embryos and planetesimals and thus, the results are globally similar to those found in the previous work.
Related Links	http://arxiv.org/abs/1409.7041 https://www.cambridge.org/core/services/aop-cambridge-core/content/view/61A3971CC4C65FA6FAB63D14A5D71AC4/S174392131400831Xa.pdf/div-class-title-terrestrial-planet-formation-in-low-mass-disks-dependence-with-initial-conditions-div.pdf
Ending Page	219
Page Count	2
Starting Page	218
ISSN	17439213
e-ISSN	17439221
DOI	10.1017/s174392131400831x
Journal	Proceedings of the International Astronomical Union
Issue Number	S310
Volume Number	9
Language	English
Publisher	Cambridge University Press (CUP)
Publisher Date	2014-07-01
Access Restriction	Open
Subject Keyword	Proceedings of the International Astronomical Union Astronomy and Astrophysics Planetary Systems Terrestrial Planets body Simulations
Content Type	Text
Resource Type	Article
Subject	Astronomy and Astrophysics Space and Planetary Science