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Table 3

Properties of the central ionized core of M 2-9 derived from our radiative transfer modeling (Sect. 6.1 and Fig. 6).

Input parameters
Distance (d) 650pc (*)
LSR Systemic velocity (Vsys) +78 km s−1
Geometry C-shaped horn(†)
Inclination (i) 12°
Equatorial radius (Req ) 8 au
Outer radius (Rout) 40 au
Nucleus outer radius (R0) 4 au
HVSs inner boundary (y1) 15au
HVSs outer boundary (y2) 28 au
Electron temperature (Te) 15 000 K
Electron density (ne):
  nucleus (I) 2.5×108 cm−3
  inner wind (II) 1.7×108(r4au)3.0cm3${1.7 \times {{10}^8}{{\left( {{r \over {4{\rm{au}}}}} \right)}^{ - 3.0}}{\rm{c}}{{\rm{m}}^{ - 3}}}$
  HVSs (III) 1.0×108(r15at)4.7cm3${1.0 \times {{10}^8}{{\left( {{r \over {15{\rm{uat}}}}} \right)}^{ - 4.7}}{\rm{c}}{{\rm{m}}^{ - 3}}}$
  outer wind (IV) 2.5×106(r28au)1.4cm3${2.5 \times {{10}^6}{{\left( {{r \over {28{\rm{au}}}}} \right)}^{ - 1.4}}{\rm{c}}{{\rm{m}}^{ - 3}}}$
Kinematics radial expansion + rotation
Expansion velocity (Vexp ):
  nucleus (I) 10 km s−1
  inner wind (II) 10 km s−1
  HVSs (III) 70+1.5×(r -15 au)km s−1
  outer wind (IV) 90 km s−1
Rotation velocity (Vrot) 7–10 km s−1
Implied physical properties of the jet
Ionized mass (Mion) 4.3×10−6 M
Mass-loss rate () 7.2×10−7 M yr−1
Kinematic age (Tkin ) 1.0–10.3 yr (~6 yr)
Scalar momentum (P) (‡) 6.4×1034 g cm/s
Total kinetic energy (Ek) 2.8×1041 erg
Mechanical luminosity (× Vexp) 1.5×1033 erg/s

Notes. In all cases, r is the radial distance to the center. Departure coefficients bn are from (Storey & Hummer 1995). Regions I-IV within the wind are shown in Fig. 6. The model presented has 3333 cubic cells of 0.″0015×0.″0015×0.″0015 (~1 au×1 au×1 au).(*) Adopted (see Sect. 1). (†)See Fig. 6 for details.(‡) Linear momentum defined as a “scalar” magnitude computed as the sum of the momentum moduli for every cell as defined in Bujarrabal et al. (2001).

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