Table B.3.
HST/ACS F850LP mass MGE model assuming a varying stellar M*/L and varying IMF.
j |
![]() |
log (Σj) | σj | qj | Ψj |
---|---|---|---|---|---|
(M⊙) | (M⊙ pc−2) | (arcsec) | (deg) | ||
(1) | (2) | (3) | (4) | (5) | (6) |
1 | 7.013 | 5.262 | 0.037 | 1.0 | 90.00 |
2 | 7.619 | 5.204 | 0.08 | 1.0 | 90.00 |
3 | 8.033 | 5.339 | 0.126 | 0.77 | 88.64 |
4 | 7.862 | 4.657 | 0.262 | 0.57 | 74.5 |
5 | 8.335 | 4.282 | 0.568 | 0.86 | 71.65 |
6 | 8.467 | 3.659 | 1.304 | 0.93 | 74.26 |
7 | 8.402 | 3.126 | 2.209 | 0.96 | -27.53 |
8 | 8.197 | 2.684 | 4.053 | 0.49 | -34.0 |
9 | 8.672 | 2.864 | 4.221 | 0.89 | 47.89 |
10 | 8.754 | 2.543 | 7.219 | 0.77 | -38.1 |
11 | 8.838 | 2.278 | 9.532 | 0.99 | -0.62 |
12 | 9.31 | 2.208 | 21.6 | 0.67 | -36.66 |
13 | 9.133 | 1.338 | 56.037 | 0.49 | -30.62 |
14 | 9.563 | 1.458 | 56.037 | 1.0 | -63.69 |
Notes. Column 1: Index of the Gaussian component. Column 2: Mass of Gaussian component derived with the constant dynamical M*/L = 0.86 M⊙/L⊙ from the Schwarzschild modelling. Column 3: Surface mass density. Column 4: Gaussian width along the axis. Column 5: Axial ratio for each Gaussian component. Column 6: Position angle for each Gaussian component. The stellar mass of the galaxy based on this MGE is 1.0 × 1010 M⊙.
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