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Home All issues Volume 500 / No 3 (June IV 2009) A&A, 500 3 (2009) 1249-1252 Full HTML
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Table 1:

Results of the formation of a Jupiter-like planet, where the accreted planetesimals have a radius of 100 kma.
Disc density Previous results New results
[MMSN] Cross- over time [My] Cross- over mass [ ${M_{\oplus}}$] Cross- over time [My] Cross- over mass [ ${M_{\oplus}}$]
$\; \; 6$ 11.40 $\; \; 44.70$ 7.20 $\; \;25.50$
$\; \; 7$ $\; \; 8.75$ $\; \; 55.40$ 5.58 $\; \; 27.90$
$\; \; 8$ $\; \; 7.00$ $\; \; 66.60$ 4.60 $\; \; 29.30$
$\; \; 9$ $\; \; 5.70$ $\; \; 77.60$ 3.78 $\; \;30.90$
10 $\; \; 4.80$ $\; \; 88.50$ 3.20 $\; \;31.90$
a The first column indicates the disc density in terms of the MMSN, the second and third columns show the results corresponding to Paper I, and the last two columns list the updated results for exactly the same conditions but with the corrected interpolation formulae for the SCVH's EOS for a mixture of hydrogen and helium.

Source LaTeX | All tables | In the text

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