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Table 2
Photometry of the triple system: estimate of the IR flux excess from the apparent magnitudes, the estimated extinction and the spectral type for GG Tau Aa and for the close binary Ab1–Ab2.
A V | I | J | H | K s | L′ | ||||||||
mag | σ | mag | σ | mag | σ | mag | σ | mag | σ | ||||
|
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Aa (observed)a | 0.30 | 10.46 | 0.02 | 9.24 | 0.21 | 8.27 | 0.25 | 7.73 | 0.16 | 6.72 | 0.13 | ||
Aa (dereddened)b | 10.26 | 9.14 | 8.21 | 7.69 | 6.81 | ||||||||
Aa (M0V)c | 10.26 | 9.26 | 8.63 | 8.46 | 8.32 | ||||||||
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Fexcess/Ftotd | 0 | 0.10 | 0.17 | 0.32 | 0.16 | 0.51 | 0.07 | 0.75 | 0.03 | ||||
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Ab1+Ab2 (obs.)a | 0.45 | 12.19 | 0.04 | 10.12 | 0.21 | 9.07 | 0.32 | 8.53 | 0.24 | 7.69 | 0.04 | ||
Ab1+Ab2 (dered.)b | 11.89 | 9.97 | 8.98 | 8.47 | 7.66 | ||||||||
Ab1 (M2V)c | 12.16 | 11.01 | 10.31 | 10.11 | 9.95 | ||||||||
Ab2 (M3.5V)c | 13.53 | 12.13 | 11.48 | 11.23 | 11.02 | ||||||||
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![]() ![]() |
2.1 | 1.9 | 1.9 | 1.8 | 1.7 | ||||||||
![]() ![]() |
3.5 | 2.8 | 2.9 | 2.8 | 2.7 | ||||||||
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Fexcess/Ftot (M2/M3)d | 0 | 0.48 | 0.10 | 0.61 | 0.12 | 0.70 | 0.07 | 0.83 | 0.02 |
Notes.
(a)
Spatially resolved apparent magnitudes from Hartigan & Kenyon (2003),
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