Table 3
Parameter limits from the ten best Robitaille fits for sources B-1, B-2, and B-3.
Source | Stellar M (M⊙) | Stellar T (K) | L (L⊙) | ||||||
Min | Best | Max | Min | Best | Max | Min | Best | Max | |
|
|||||||||
B-1 | 1.61 | 1.71 | 1.94 | 4581 | 5612 | 5612 | 4.72 | 5.08 | 6.46 |
B-2 | 0.80 | 3.07 | 3.99 | 4091 | 5101 | 11582 | 7.02 | 18.7 | 121 |
B-3 | 0.10 | 0.13 | 0.13 | 2835 | 2954 | 2960 | 0.12 | 0.20 | 0.24 |
B-3 (NIR–MIR) free D | 0.23 | 0.23 | 0.23 | 3168 | 3168 | 3181 | 0.35 | 0.38 | 0.39 |
Notes. B-1, B-2 and B-3 are fitted with a strict distance limit (126–154 pc). B-3 (NIR–MIR) free D is fitted with only NIR–MIR points, with a free distance range 20–800 pc, leading to distance estimates of 174–182 pc.
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