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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 2:

The same as in Table 1 but considering that the radius of the accreted planetesimals is 10 km.
Disc density Previous results New results
[MMSN] Cross- over time [My] Cross- over mass [ ${M_{\oplus}}$] Cross- over time [My] Cross- over mass [ ${M_{\oplus}}$]
$\; \; 6$ $\; \; 4.95$ $\; \; 46.70$ 2.43 $\; \; 31.80$
$\; \; 7$ $\; \; 3.53$ $\; \; 58.70$ 1.97 $\; \; 34.80$
$\; \; 8$ $\; \; 2.65$ $\; \; 71.40$ 1.49 $\; \; 36.80$
$\; \; 9$ $\; \; 2.00$ $\; \; 84.85$ 1.32 $\; \;38.60$
10 $\; \; 1.65$ $\; \;99.00$ 1.10 $\; \; 39.90$

Source LaTeX | All tables | In the text

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