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Overcoming migration during giant planet formation | | E. W. Thommes
; L. Nilsson
; N. Murray
; | | Date: |
16 Jan 2007 | | Abstract: | In the core accretion model, gas giant formation is a race between growth and migration; for a core to become a jovian planet, it must accrete its envelope before it spirals into the host star. We use a multizone numerical model to extend our previous investigation of the "window of opportunity" for gas giant formation within a disk. When the collision cross-section enhancement due to core atmospheres is taken into account, we find that a broad range of protoplanetary disks posses such a window. | | Source: | arXiv, astro-ph/0701443 | | Services: | Forum | Review | PDF | Favorites | |
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