Unveiling the traits of massive young stellar objects through a multi-scale survey

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Table 1

MYSOs included in this study with a column stating whether VISIR or COMICS data were used in the fitting process.

Name	RA (J2000)	Dec (J2000)	log	Distance	VISIR (V) or COMICS (C)?
	(h:m:s)	(d:m:s)		(kpc)
G305.20+0.21	13:11:10.45	–62:34:38.6	4.7 ⁽¹⁾	4.0 ⁽²⁾	V
W33A	18:14:39.0	–17:52:03	4.5 ⁽³⁾	2.4 ⁽⁴⁾	C
NGC 2264 IRS1	06:41:10.15	+09:29:33.6	3.6 ⁽⁵⁾	0.7 ⁽⁶⁾	C
S255 IRS3	06:12:54.02	17:59:23.60	4.7 ⁽⁷⁾	1.8 ⁽⁸⁾	C
Mon R2 IRS2	06:07:45.8	–06:22:53.2	3.8 ⁽⁹⁾	0.8 ⁽¹⁰⁾	C
IRAS 17216-3801	17:25:06.51	–38:04:00.4	4.8 ⁽¹¹⁾	3.1 ⁽¹²⁾	V
M8EIR	18:04:53.18	–24:26:41.4	3.8 ⁽¹³⁾	1.3 ⁽¹⁴⁾	C
AFGL 2136	18:22:26.38	–13:30:12.0	5 ⁽¹⁾	2.2 ^{(15), (16)}	C

References. (1) Lumsden et al. (2013); (2) Mottram et al. (2011); (3) (Mottram et al. 2011); (4) Immer et al. (2013); (5) Grellmann et al. (2011); (6) Kamezaki et al. (2014); (7) (Wang et al. 2011); (8) Burns et al. (2016); (9) Henning et al. (1992); (10) Herbst & Racine (1976); (11) Kraus et al. (2017); (12) Boley et al. (2013); (13) Linz et al. (2009); (14) Damiani et al. (2019); (15) Urquhart et al. (2012); (16) Urquhart et al. (2014).

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