EDP Sciences logo
Subscriber Authentication Point
Search
Menu
Home All issues Volume 510 (February 2010) A&A, 510 (2010) A18 Full HTML
Free Access

   

Table 5:

Results for the fine structure emission lines from various disk models and test runs.
    O  I 63 $\mu $m O  I 145 $\mu $m C  II 157.7 $\mu $m
$M_{\rm disk}$ Model $F_{\rm line}$ $F_{\rm cont}$ Peak sep. $F_{\rm line}$ $F_{\rm cont}$ Peak sep. $F_{\rm line}$ $F_{\rm cont}$ Peak sep.
$[M_\odot]$   [10-18 W/m2] [Jy] [km s-1] [10-18 W/m2] [Jy] [km s-1] [10-18 W/m2] [Jy] [km s-1]
$2.2 \times 10^{-2}$ MC 1.93(3) 1.44(2) 1.9 2.13(2) 1.25(2) 2.6 5.39(1) 1.14(2) 2.2
10-2 MC 1.29(3) 1.03(2) 2.4 1.18(2) 6.57(1) 3.0 4.69(1) 5.91(1) 2.2
10-3 MC 6.57(2) 2.58(1) 2.5 3.89(1) 8.84 5.9 2.98(1) 7.69 2.2
10-4 MC 2.65(2) 4.56 5.9 8.06 9.09(-1) 6.2 1.40(1) 1.01 2.4
10-5 MC 4.19(1) 9.89(-1) 7.7 1.11 1.72(-1) 6.0 4.53 2.71(-1) 2.3
10-6 MC 1.99 1.50(-1) 12.2 5(-2) 3(-2) 10.3 2.77 1.43(-1) 2.2
10-2 LTE 2.25(3) 1.05(2) 2.2 1.30(2) 6.63(1) 2.7 5.22(1) 5.96(1) 2.2
10-2 ES 1.27(3) 1.05(2) 2.3 1.23(2) 6.63(1) 2.9 4.93(1) 5.96(1) 2.2
10-2 no O  I >2000 K 1.29(3) 1.03(2) 2.4 1.18(2) 6.57(1) 3.0      
10-2 $R_{\rm in,out}=0.5,500$ AU 1.23(3) 1.06(2) 2.6 1.14(2) 6.16(1) 3.2 2.26(1) 5.41(1) 2.7
10-2 $R_{\rm in,out}=0.5,300$ AU 9.40(2) 1.01(2) 3.3 8.99(1) 4.98(1) 4.0 7.33 4.66(1) 3.5
10-2 $R_{\rm in,out}=0.5,100$ AU 5.74(2) 8.27(1) 5.6 4.18(1) 3.19(1) 6.0 1.35 2.76(1) 6.3
10-2 $R_{\rm in,out}=0.5,30$ AU 2.40(2) 5.03(1) 11.2 1.26(1) 1.47(1) 11.4      
10-2 $R_{\rm in,out}=30,100$ AU 3.70(2) 3.42(1) 5.5 3.08(1) 1.75(1) 6.1      
10-2 $R_{\rm in,out}=30,700$ AU 1.11(3) 6.13(1) 2.5 1.08(2) 5.29(1) 3.0 4.64(1) 4.82(1) 2.2
10-2 $R_{\rm in,out}=100,700$ AU             4.59(1) 3.31(1) 2.2
10-2 $T_{\rm eff}=9500$ K 5.53(3) 1.68(2) 2.8 4.56(2) 8.60(1) 2.9 1.50(2) 7.63(1) 2.3
10-2 $T_{\rm eff}=10500$ K 9.03(3) 1.78(2) 3.1 6.75(2) 8.85(1) 2.8 3.17(2) 7.84(1) 2.3
10-2 $a_{\rm min,max}=0.01,1~\mu$m 6.48(2) 1.42(2) 2.3 3.24(1) 3.53(1) 2.5 6.30(1) 2.85(1) 2.2
10-2 $a_{\rm min,max}=1,200~\mu$m 3.22(3) 1.44(2) 2.7 3.17(2) 7.21(1) 3.2 2.39(1) 6.42(1) 2.2

Notes. In the model column, MC, LTE and ES denote the use of level populations from Monte Carlo line radiative transfer, LTE and escape probability, respectively. Line and continuum fluxes are shown for a distance of 131 pc and an inclination of 45 degrees. Numbers in parentheses indicate powers of ten, i.e. 1.93(3) denotes $1.93 \times 10^3$. The peak separation is defined as the distance between the two maxima in the double peaked line profile measured in km s-1.


Source LaTeX | All tables | In the text

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.