![]() ![]() |
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t | R (AU) | ||||||||||||||
(Myr) | 10 | 30 | 100 | 10 | 30 | 100 | 10 | 30 | 100 | 10 | 30 | 100 | |||
M0=0.20,
![]() |
M0=0.50,
![]() |
M0=1.0,
![]() |
M0=5.0,
![]() |
||||||||||||
1.0 | 19.7 | 20.1 | 21.5 | 6.7 | 6.0 | 5.5 | 7.6 | 3.8 | 1.9 | 17.0 | 2.9 | 0.4 | |||
1.6 | 21.1 | 21.3 | 22.2 | 6.1 | 5.8 | 5.7 | 5.3 | 3.4 | 2.3 | 23.0 | 3.9 | 0.4 | |||
3.1 | 22.9 | 23.0 | 23.4 | 5.9 | 5.8 | 5.9 | 3.3 | 2.6 | 2.2 | 24.6 | 4.4 | 0.6 | |||
![]() ![]() |
|||||||||||||||
t | R (AU) | ||||||||||||||
(Myr) | 10 | 30 | 100 | 10 | 30 | 100 | 10 | 30 | 100 | 10 | 30 | 100 | |||
M0=0.20,
![]() |
M0=0.50,
![]() |
M0=1.0,
![]() |
M0=5.0,
![]() |
||||||||||||
1.0 | ... | ... | ... | 32.1 | 32.3 | 33.8 | 17.4 | 16.0 | 15.1 | 54.1 | 9.3 | 1.2 | |||
1.6 | ... | ... | ... | 33.3 | 33.5 | 34.4 | 16.4 | 15.7 | 15.4 | 37.5 | 9.7 | 2.2 | |||
3.1 | ... | ... | ... | 35.1 | 35.3 | 35.7 | 16.0 | 15.8 | 15.8 | 16.5 | 6.1 | 3.3 | |||
![]() ![]() |
|||||||||||||||
t | R (AU) | ||||||||||||||
(Myr) | 10 | 30 | 100 | 10 | 30 | 100 | 10 | 30 | 100 | 10 | 30 | 100 | |||
M0=0.20,
![]() |
M0=0.50,
![]() |
M0=1.0,
![]() |
M0=5.0,
![]() |
||||||||||||
1.0 | 2.1 | 1.9 | 1.6 | 2.6 | 1.3 | 0.6 | 4.4 | 1.3 | 0.3 | 5.4 | 1.1 | 0.2 | |||
1.6 | 1.8 | 1.7 | 1.6 | 1.7 | 1.0 | 0.5 | 2.9 | 1.1 | 0.4 | 5.1 | 1.2 | 0.2 | |||
3.1 | 1.6 | 1.5 | 1.5 | 1.0 | 0.6 | 0.4 | 1.5 | 0.6 | 0.3 | 8.5 | 0.5 | 0.02 | |||
![]() ![]() |
|||||||||||||||
t | R (AU) | ||||||||||||||
(Myr) | 10 | 30 | 100 | 10 | 30 | 100 | 10 | 30 | 100 | 10 | 30 | 100 | |||
M0=0.20,
![]() |
M0=0.50,
![]() |
M0=1.0,
![]() |
M0=5.0,
![]() |
||||||||||||
1.0 | 12.1 | 12.0 | 12.0 | 5.3 | 4.4 | 3.6 | 6.2 | 3.3 | 1.7 | 19.3 | 3.9 | 0.6 | |||
1.6 | 12.0 | 12.0 | 12.0 | 4.5 | 4.0 | 3.6 | 4.5 | 2.6 | 1.6 | 14.6 | 3.3 | 0.7 | |||
3.1 | 12.1 | 12.1 | 12.2 | 3.7 | 3.5 | 3.3 | 2.7 | 1.7 | 1.3 | 8.6 | 2.4 | 0.8 |
Notes. The fractions are given in per cent of the total silicate dust abundance at the indicated distance from the star (R) and time after the onset of collapse (t). The initial cloud core mass (M0, in )
and the disk mass at the end of the accretion phase (
,
in
)
are listed for each combination of parameters.
(a) No disk is formed at all for this combination of parameters.
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