SABOCA 350-μm and LABOCA 870-μm dust continuum imaging of IRAS 05399-0121: mapping the dust properties of a pre- and protostellar core system

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Table 3

Results of SED modelling of IRAS 05399-0121.

Parameter	Value^a

Min. χ²/N_data	103.6^+ 36.3
Inclination, i [°]	31.8^+ 17.7
Visual extinction, A_V [mag]
Stellar age, τ_⋆ [10³ yr]
Stellar mass, M_⋆ [M_⊙]	0.46^+ 1.09
Stellar temperature, T_⋆ [10³ K]	3.65^+ 0.53
Envelope accretion rate, Ṁ_env [10^-5M_⊙ yr^-1]
Disk mass, M_disk [M_⊙]
Circumstellar extinction, [mag]
Total luminosity, L_tot [L_⊙]
Envelope mass, M_env [M_⊙]
Stage	I

Notes.

^(a)

For each model parameter, the best-fit value is given with the ± errors computed from the minimum and maximum values obtained from the three next-best model fits. For some parameters, the best-fit value is the lowest one.

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