Direct detection of the tertiary component in the massive multiple HD 150136 with VLTI

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Table 1

Best-fit parameters of a binary model (inner system plus tertiary) for HD 150136 to the closure phases of all bands combined and of each band individually.

Parameter	Combined	J	H	K

f_inner^a	0.80	0.78	0.80	0.82
f_T^b	0.20	0.22	0.20	0.18
d [mas]^c	7.27	7.27	7.19	7.19
Φ [deg]^d	209.0	210.2	206.7	210.7

Notes.

^(a)

Fraction of total flux contained in the inner system (P+S).

^(b)

Fraction of total flux contained in the tertiary (T).

^(c)

Angular separation between inner system and T in milliarcseconds.

^(d)

Projected angle of the system on the sky.

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