Cabral, N.; Fouchet, L.; Alibert, Y.; Mordasini, C.; Benz, W. (2010). Irradiated disks and planet population synthesis. In: Boissier, S; Heydari-Malayeri, M; Samadi, R; Valls-Gabaud, D (eds.) Annual meeting of the French Society of Astronomy and Astrophysics. Marseille, France. 1 - 24 June 2010.
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2010sf2a.conf..0281C.pdf - Accepted Version Available under License BORIS Standard License. Download (1MB) | Preview |
Recent planet population synthesis models (Alibert et al. 2010, submitted) have emphasized the key role played by the proto-planetary disk properties in determining the overall planet population characteristics. We present a disk model that takes into account viscous heating and irradiation by a central star. We consider the case of an equilibrium flaring angle. We illustrate the consequences of the resulting changes in the disk structure on the planet population by the synthetic populations corresponding to each of the different structures.
Item Type: |
Conference or Workshop Item (Paper) |
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Division/Institute: |
08 Faculty of Science > Physics Institute |
UniBE Contributor: |
Alibert, Yann Daniel Pierre, Benz, Willy |
Language: |
English |
Submitter: |
Factscience Import |
Date Deposited: |
04 Oct 2013 14:16 |
Last Modified: |
05 Dec 2022 14:04 |
Related URLs: |
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Uncontrolled Keywords: |
planetary systems: formation, protoplanetary disks, planets and satellites: formation |
BORIS DOI: |
10.7892/boris.4830 |
URI: |
https://boris.unibe.ch/id/eprint/4830 (FactScience: 209464) |
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