Open Access
Table 2
XRISM Resolve best-fit iron abundance values for 1T, 2T, and gdem models with (✓) and without (✗) the RS for the inner (rin) and outer shells (rout) as defined in the caption of Fig. 6.
RS | rin 3D | 1T | 2T | gdem | rout 3D | 1T | 2T | gdem | |
---|---|---|---|---|---|---|---|---|---|
A2029 | ✗ | 0.86 | 0.70 ± 0.01 | − | 0.72 ± 0.01 | 0.65 | 0.55 ± 0.01 | − | 0.56 ± 0.01 |
✓ | 0.86 | 0.66 ± 0.01 | − | 0.68 ± 0.01 | 0.65 | 0.54 ± 0.01 | − | 0.56 ± 0.01 | |
A1795 | ✗ | 0.86 | 0.76 ± 0.01 | 0.75 ± 0.01 | 0.73 ± 0.01 | 0.68 | 0.59 ± 0.01 | − | 0.59 ± 0.01 |
✓ | 0.86 | 0.73 ± 0.01 | 0.70 ± 0.01 | 0.69 ± 0.01 | 0.68 | 0.58 ± 0.01 | − | 0.58 ± 0.01 | |
A383 | ✗ | 0.65 | 0.65 ± 0.02 | − | 0.63 ± 0.02 | 0.41 | 0.36 ± 0.02 | − | 0.36 ± 0.02 |
✓ | 0.65 | 0.62 ± 0.02 | − | 0.61 ± 0.02 | 0.41 | 0.37 ± 0.02 | − | 0.37 ± 0.02 | |
Perseus | ✗ | 0.85 | 0.83 ± 0.004 | − | 0.82 ± 0.004 | 0.87 | 0.81 ± 0.003 | 0.80 ± 0.003 | 0.80 ± 0.003 |
✓ | 0.85 | 0.75 ± 0.004 | − | 0.73 ± 0.004 | 0.87 | 0.75 ± 0.003 | 0.75 ± 0.003 | 0.74 ± 0.004 | |
A262 | ✗ | 0.87 | 0.72 ± 0.02 | − | 0.80 ± 0.02 | 0.81 | 0.67 ± 0.01 | − | 0.67 ± 0.01 |
✓ | 0.87 | 0.69 ± 0.01 | − | 0.77 ± 0.02 | 0.81 | 0.66 ± 0.01 | − | 0.66 ± 0.01 | |
NGC 4636 | ✗ | 0.84 | 0.40 ± 0.01 | 0.73 ± 0.04 | 0.88 ± 0.04 | 0.88 | 0.80 ± 0.03 | 0.87 ± 0.04 | 0.88 ± 0.04 |
✓ | 0.84 | 0.32 ± 0.01 | 0.59 ± 0.03 | 0.69 ± 0.03 | 0.88 | 0.81 ± 0.03 | 0.89 ± 0.03 | 0.92 ± 0.04 |
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