Disc kinematics and stability in high-mass star formation - Linking simulations and observations

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Volume 632 (December 2019)

A&A, 632 (2019) A50

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Table 2

Summary of temperatures, masses, and Q values for the synthetic observations.

Interferometer	Distance	Inclination	Median T^(a)	Median	Mass^(c)	Median Q
	(pc)	(degrees)	(K)	(K)	(M_⊙)
ALMA	800	10	115	228	2.9	2.6
	800	30	112	213	3.2	2.3
	800	60	110	204	3.3	1.5
	800	80	110	202	2.8	0.5

ALMA	2000	10	112	214	2.9	3.5
	2000	30	111	211	3.0	3.1
	2000	60	108	187	3.0	2.0
	2000	80	108	173	2.5	0.7

NOEMA	800	10	121	153	2.6	5.2
	800	30	118	145	2.7	4.7
	800	60	115	142	2.6	3.1
	800	80	114	139	2.4	1.0

NOEMA	2000	10	125	148	3.5	3.6
	2000	30	125	146	3.4	3.4
	2000	60	123	143	3.3	2.0
	2000	80	119	143	2.9	0.5

Notes. ^(a) Median temperature, calculated from the maps presented in Fig. 8. ^(b) Median temperature within 12σ dust continuum (second outermost) contours, as presented in Fig. 8. ^(c) Mass is calculatedfrom the dust emission using Eq. (5).

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