The massive protostar W43-MM1 as seen by Herschel-HIFI water spectra: high turbulence and accretion luminosity

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Table 3

Parameters used in Whitney-Robitaille continuum model and derived physical quantities.


Parameter used		Derived parameter

Inner radius (AU)^a	100	Mass (M_⊙)	3520
Outer radius (AU)^a	55 000	T_out (K)	19
Distance (kpc)	5.5	T_in (K)	1377
Luminosity (L_⊙)	2.3 × 10⁴
Density exponent	−1.5

Notes.

^(a)

Motte et al. (2003).

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