Infall, outflow, and rotation in the G19.61-0.23 hot molecular core

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Table 3

Results of submm continuum emission observations.

Name	Peak Position (J2000)		I _890 μm ^a	S _890 μm ^b	D _d ^c	R _d ^d	M _d ^e
	RA(hh:mm:ss)	Dec(dd:mm:ss)	(Jy beam^-1)	(Jy)	(arcsec)	(pc)	(M_⊙)

SMA1	18:27:38.069	−11:56:37.30	1.89	3.2	2.4	0.072	1300
SMA2	18:27:38.021	−11:56:38.75	0.29	0.52	1.5	0.045	220
SMA3	18:27:37.955	−11:56:35.08	0.25	0.15	0.81	0.025	60

Notes.

^(a)

Peak intensity. The uncertainty may be given by the 3σ level of the image noise level, i.e., 0.1 Jy beam^-1.

^(b)

Flux density, see Sect. 3.1.2.

^(c)

Effective diameter of the submm emission, which is given by where A is the area enclosed by the 5σ level contour enclosing each source. Note that, at SMA2 and SMA3, the 5σ level corresponds to the 61% and 71% levels with respect to their peak intensities, respectively.

^(d)

Effective radius of the submm emission.

^(e)

Mass of the core estimated from the flux S_890 μm in Col. 5, assuming β = 1 and a dust temperature of 80 K.

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