A binary engine fuelling HD 87643's complex circumstellar environment - Determined using AMBER/VLTI imaging

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Table 4:

Estimated fluxes for each component from the model fitting of Sect. 2.1.2.
Band or $\lambda$	Primary	Background	Secondary
(total value)	(W/m²/ $\mu$ m)	(W/m²/ $\mu$ m)	(W/m²/ $\mu$ m)
H (4.8 mag)	$8.5\times10^{-12}$	$1.6\times10^{-12}$	$3.7\times10^{-12}$
K (3.5 mag)	$1.2\times10^{-11}$	$1.5\times10^{-12}$	$3.1\times10^{-12}$
8.1 $\mu$ m (92 Jy)	$7.2\times10^{-13}$	$2.9\times10^{-12}$	$5.9\times10^{-13}$
10.5 $\mu$ m (146 Jy)	$3.5\times10^{-13}$	$3.0\times10^{-12}$	$6.0\times10^{-13}$
12.9 $\mu$ m (126 Jy)	$1.4\times10^{-13}$	$1.7\times10^{-12}$	$4.3\times10^{-12}$

We used 2MASS magnitudes as the total magnitude in H and K-band and the MIDI fluxes in N-band.

Source LaTeX | All tables | In the text

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