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J/A+A/490/151/table1
Post annotation
Photometric evolution of star clusters models (Kruijssen+, 2008)
*Fitting values for a, b and c for the luminous fractional cluster mass decrease due to stellar evolution. (10 rows) (Note)
 
Full

Type

Z

Mass
solMass
aS

bS

cS

aK

bK

cK

Dir

1L 0.000468.5101 6.83 0.316-1.824 6.84 0.298-1.648Z0004
2L 0.004069.8779 6.80 0.313-1.844 6.80 0.295-1.667Z004
3L 0.008071.6802 6.76 0.309-1.853 6.77 0.291-1.674Z008
4L 0.020068.1211 6.70 0.308-1.872 6.71 0.290-1.691Z02
5L 0.050049.4481 6.63 0.314-1.897 6.65 0.297-1.714Z05
6T 0.000468.5101 6.93 0.271-1.855 6.93 0.255-1.682Z0004
7T 0.004069.8779 6.89 0.271-1.872 6.90 0.256-1.696Z004
8T 0.008071.6802 6.88 0.265-1.877 6.88 0.250-1.701Z008
9T 0.020068.1211 6.82 0.263-1.893 6.83 0.248-1.716Z02
10T 0.050049.4481 6.78 0.263-1.908 6.79 0.249-1.731Z05
The 1 column in color are computed by VizieR, and are not part of the original data.
J/A+A/490/151/models
Post annotation
Photometric evolution of star clusters models (Kruijssen+, 2008)
Summary of models (3140 rows)
 
Full

File

Z

IMF

r

L

tD
Myr
logMo
[solMass]
logMf
[solMass]
logtf
[yr]
Dir

Record

Plot

1K0000_01.dat 0.0004S-- 1 2.279 2.001 7.062Z0004 42Plot
2K0000_01.dat 0.0004S-- 1 2.465 2.009 7.359Z0004 54Plot
3K0000_01.dat 0.0004S-- 1 2.651 2.006 7.580Z0004 109Plot
4K0000_01.dat 0.0004S-- 1 2.837 2.007 7.760Z0004 196Plot
5K0000_01.dat 0.0004S-- 1 3.023 2.000 7.919Z0004 309Plot
6K0000_01.dat 0.0004S-- 1 3.209 2.035 8.057Z0004 445Plot
7K0000_01.dat 0.0004S-- 1 3.395 2.017 8.195Z0004 601Plot
8K0000_01.dat 0.0004S-- 1 3.581 2.070 8.319Z0004 777Plot
9K0000_01.dat 0.0004S-- 1 3.767 2.086 8.443Z0004 971Plot
10K0000_01.dat 0.0004S-- 1 3.953 2.040 8.568Z0004 1183Plot
11K0000_01.dat 0.0004S-- 1 4.140 2.073 8.685Z0004 1413Plot
12K0000_01.dat 0.0004S-- 1 4.326 2.061 8.803Z0004 1660Plot
13K0000_01.dat 0.0004S-- 1 4.512 2.254 8.913Z0004 1924Plot
14K0000_01.dat 0.0004S-- 1 4.698 2.161 9.030Z0004 2204Plot
15K0000_01.dat 0.0004S-- 1 4.884 2.338 9.141Z0004 2501Plot
16K0000_01.dat 0.0004S-- 1 5.070 2.509 9.251Z0004 2814Plot
17K0000_01.dat 0.0004S-- 1 5.256 2.147 9.369Z0004 3143Plot
18K0000_01.dat 0.0004S-- 1 5.442 2.297 9.479Z0004 3489Plot
19K0000_01.dat 0.0004S-- 1 5.628 2.444 9.590Z0004 3851Plot
20K0000_01.dat 0.0004S-- 1 5.814 2.587 9.700Z0004 4229Plot
21K0000_01.dat 0.0004S-- 1 6.000 2.725 9.811Z0004 4623Plot
22K0000_01.dat 0.0004S-- 1 6.186 2.854 9.921Z0004 5033Plot
23K0000_01.dat 0.0004S-- 1 6.372 2.96310.032Z0004 5459Plot
24K0000_01.dat 0.0004S-- 1 6.558 3.04810.142Z0004 5901Plot
25K0000_01.dat 0.0004S-- 1 6.744 3.08010.253Z0004 6359Plot
26K0000_01.dat 0.0004S-- 1 6.930 5.56610.274Z0004 6833Plot
27K0000_03.dat 0.0004S-- 3 2.279 2.004 7.511Z0004 42Plot
28K0000_03.dat 0.0004S-- 3 2.465 2.004 7.815Z0004 119Plot
29K0000_03.dat 0.0004S-- 3 2.651 2.002 8.036Z0004 240Plot
30K0000_03.dat 0.0004S-- 3 2.837 2.004 8.216Z0004 393Plot
31K0000_03.dat 0.0004S-- 3 3.023 2.002 8.374Z0004 572Plot
32K0000_03.dat 0.0004S-- 3 3.209 2.038 8.512Z0004 774Plot
33K0000_03.dat 0.0004S-- 3 3.395 2.026 8.651Z0004 996Plot
34K0000_03.dat 0.0004S-- 3 3.581 2.005 8.782Z0004 1238Plot
35K0000_03.dat 0.0004S-- 3 3.767 2.003 8.906Z0004 1499Plot
36K0000_03.dat 0.0004S-- 3 3.953 2.069 9.024Z0004 1778Plot
37K0000_03.dat 0.0004S-- 3 4.140 2.101 9.141Z0004 2074Plot
38K0000_03.dat 0.0004S-- 3 4.326 2.088 9.258Z0004 2387Plot
39K0000_03.dat 0.0004S-- 3 4.512 2.260 9.369Z0004 2717Plot
40K0000_03.dat 0.0004S-- 3 4.698 2.159 9.486Z0004 3063Plot
41K0000_03.dat 0.0004S-- 3 4.884 2.325 9.597Z0004 3426Plot
42K0000_03.dat 0.0004S-- 3 5.070 2.489 9.707Z0004 3805Plot
43K0000_03.dat 0.0004S-- 3 5.256 2.136 9.825Z0004 4200Plot
44K0000_03.dat 0.0004S-- 3 5.442 2.275 9.935Z0004 4612Plot
45K0000_03.dat 0.0004S-- 3 5.628 2.40010.046Z0004 5040Plot
46K0000_03.dat 0.0004S-- 3 5.814 2.50610.156Z0004 5484Plot
47K0000_03.dat 0.0004S-- 3 6.000 2.58010.267Z0004 5944Plot
48K0000_03.dat 0.0004S-- 3 6.186 4.91410.274Z0004 6420Plot
49K0000_03.dat 0.0004S-- 3 6.372 5.50210.274Z0004 6897Plot
50K0000_03.dat 0.0004S-- 3 6.558 5.89010.274Z0004 7374Plot
Result truncated to 50 rows
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