Jet formation in post-AGB binaries - Confronting cold magnetohydrodynamic disc wind models with observations

Open Access

Fig. 4.

Blackbody temperatures derived from the accretion disc’s spectral slope, considering either the full spectrum ( $T_{full}^{BB}$ $T^{\mathrm{BB}}_{\mathrm{full}}$ , red diamonds), or only the H band ( $T_{H}^{BB}$ $T^{\mathrm{BB}}_{\mathrm{H}}$ , blue dots). The orange shaded area denotes the ±1σ region of the T_disc estimate for IRAS 08544−4431 by Hillen et al. (2016), around which the $T_{H}^{BB}$ $T^{\mathrm{BB}}_{\mathrm{H}}$ values cluster.

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