Emergence of high-mass stars in complex fiber networks (EMERGE) - III. Fiber networks in Orion

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Table 1

General properties of the EMERGE Early ALMA Survey.

Source	Cloud	D (pc)	SF-regime	O-star	Evolutionary stage	P ⁽*⁾	P+D ⁽*⁾	P/D ⁽*⁾	ALMA Proj.ID
OMC-1	Orion A	400	High-	Yes	Evolved	36	423	0.09	2015.1.00669.S
OMC-2	Orion A	400	Intermediate-	No	Young	33	142	0.30	2015.1.00669.S
OMC-3	Orion A	400	Intermediate-	No	Young	26	102	0.34	2019.1.00641.S
OMC-4 South	Orion A	400	Low-		Evolved	11	59	0.23	2019.1.00641.S
LDN 1641N	Orion A	400	Intermediate-	No	Young	13	51	0.34	2019.1.00641.S

NGC 2023	Orion B	423	Low-	No	Young	6	8	0.75	2019.1.00641.S
Flame Nebula	Orion B	423	High-	Yes	Evolved	21	141	0.18	2019.1.00641.S

Notes. ⁽*⁾The number of protostars (P) and disks (D) here listed are merely used as reference in this paper, as they refer to larger footprints compared to our ALMA fields (see Paper I for a full discussion).

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