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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

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

Fexcess/Ftotd 0 0.10 0.17 0.32 0.16 0.51 0.07 0.75 0.03

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

/ (M2/M3)e 2.1 1.9 1.9 1.8 1.7
/ (M2/M3.5)e 3.5 2.8 2.9 2.8 2.7

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),

(b)

extinction-corrected magnitudes,

(c)

expected magnitudes from color-index and the spectral-type estimate (assuming I-band flux has a purely photospheric origin,

(d)

estimated flux excess from circumstellar material for the adopted spectral type(s),

(e)

expected flux ratios between the stellar components Ab1 and Ab2 for the given spectral types.

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