Ionization driven molecular outflow in K3-50A | Astronomy & Astrophysics (A&A)

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Table 3

K3-50A outflow properties compared to other sources.

Source	L_Bol	SiO	Molecular outflow properties
		detection	Mass	Momentum	Energy
(10⁶L_⊙)		(Y/N)	(M_⊙)	(M_⊙ km s^-1)	(10⁴⁵ erg)

K3-50A	2	Y^a^b^d	4.6	28	1.65

G10.60−0.40	1.1^c	Y^d	90^c	670^c	50^c
G10.47+0.03	1.4^c	Y^a^d	150^c	1110^c	81^c
G48.61+0.02	1.3^c	Y^e	590^c	2550^c	118^c
G19.61−0.23	1.7^c	Y^d	200^c	1740^c	150^c

Notes. Comparison with outflows from other high luminosity (>10⁶L_⊙) star forming regions. Note that the outflow properties for the comparison sources also assume optically thin emission.

Reference.

^(a)

Klaassen & Wilson (2007),

^(b)

Howard et al. (1997),

^(c)

López-Sepulcre et al. (2009),

^(d)

Klaassen & Wilson (2008),

^(e)

Klaassen et al. (2012).

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