Warm gas in protostellar outflows - II. Extremely high-velocity emission jet and outflows from OMC-2/3

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Volume 629 (September 2019)

A&A, 629 (2019) A77

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Table 7

Outflow properties derived from CO (6–5).

Velocity	δv_max ⁽¹⁾	R_max ⁽²⁾	t_d ⁽³⁾	M(H₂) ⁽⁴⁾	F_m ⁽⁵⁾	E_k ⁽⁶⁾	L_mec ⁽⁷⁾
		(10⁻²)	(10³)	(10⁻³)	(10⁻⁵)	(10⁴³)
range	(km s⁻¹)	(pc)	(yr)	(M_⊙)	(M_⊙ km s⁻¹ yr⁻¹)	(erg)	(L_⊙)
FIR 6b

Blue	8	3	4	6	2	0.7	0.02
Red	19	4	2	3	3	2	0.07
Total				9	5	2.7	0.09

FIR 6c

Blue	26	4	1	5	13	7	0.4

MMS 5

Blue	106	6	0.6	9	230	200	28
Red	59	4	0.6	5	70	30	5
Total				14	300	230	33

MMS 2

Blue	23	4	2	1	2	1	0.06
Red	19	4	2	0.4	0.5	0.3	0.01
Total				1.4	2.5	1.3	0.07

Notes. ⁽¹⁾ Maximum relative velocity of the lobe. ⁽²⁾Maximum extension of the lobe. ⁽³⁾Dynamical time. ⁽⁴⁾ H₂ mass. ⁽⁵⁾Mechanical force. ⁽⁶⁾Kinetic energy. ⁽⁷⁾Mechanical luminosity.

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