FAUST - XXV. A potential new molecular outflow in [BHB2007] 11

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Table 1

Properties of the potential new outflow in [BHB2007] 11.

Property	Value	Obtained from
Length of a single lobe, R	3300 ± 700 au	H¹³CO⁺, CCH and c-C₃H₂ PV diagrams (Fig. 3)
Expansion velocity, v_exp	2.2 ± 0.4 km s⁻¹	H¹³CO⁺, CCH and c-C₃H₂ blueshifted PV diagrams (Fig. 3)
Mass M	(1.19 ± 0.11) × 10⁻²M_⊙	C¹⁸O column density in the lobes
Dynamical timescale, t_dyn	7000 ± 1900 yr	t_dyn = R/v_exp
Mass loss rate, $\dot{M}$ $\[\dot{M}\]$	(1.7 ± 0.5) × 10⁻⁶ M_⊙ yr⁻¹	$\dot{M}$ $\[\dot{M}\]$ = M/t_dyn
Momentum injection rate, $\dot{P}$ $\[\dot{P}\]$	(3.7 ± 1.3) × 10⁻⁶M_⊙ km s⁻¹ yr⁻¹	$\dot{P} = \dot{M} v_{e x p}$ $\[\dot{P}=\dot{M} v_{exp}\]$
Kinetic energy, E	(6 ± 2) × 10⁴¹ erg	$E = \frac{1}{2} M v_{e x p}^{2}$ $\[E=\frac{1}{2} M v_{exp}^{2}\]$
Energy injection rate, $\dot{E}$ $\[\dot{E}\]$	(9 ± 4) × 10³⁷ erg yr⁻¹	$\dot{E} = E / t_{d y n}$ $\[\dot{E}=E / t_{dyn}\]$
Specific angular momentum, l	70 ± 25 au km s⁻¹	H¹³CO⁺ transversal PV diagrams in the redshifted lobe (Figs. 4, 5 and 6)
Launching radius, r₀	90 ± 30 au	H¹³CO⁺ transversal PV diagrams in the redshifted lobe (Figs. 4, 5 and 6)
SiO abundance, χ(SiO)	≥ (0.11–2.0) × 10⁻⁹	SiO, C¹⁸O and H¹³CO⁺ column density in the SiO emitting region (Fig. 2)

Notes. The quantities are corrected for the inclination of the two circumstellar disks, 40 ± 10° (Alves et al. 2019).

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