OMC 2

 

OMC-2 is a region below to OMC-3, which coincides with the Integral Shaped Filament in Orion A Molecular Cloud.

The sources named "HOPS" are the ones detected in the Herschel Orion Protostar Survey (Furlan et al. 2016), while the ones named "Source" were observed later on with VLA (Osorio et al. 2017, Díaz-Rodríguez et al. 2022).

Some VLA sources match HOPS sources and others were new findings in this Orion region.

 

 

HOPS Sources OMC-2 region

Source Lbol (L) Tbol (K) Class Number of components Other Source Names
HOPS-57 2.8 421.2 Flat 2 Source 46 1
HOPS-59 43.2 528.4 Flat 2 Source 42 1
HOPS-60 19.2 54.1 0 1 Source 39 1
HOPS-64 13.4 29.7 I 1 MIPS 2293
HOPS-66 18.3 264.9 Flat 2 Source 24 and 25 1
HOPS-70 6.0 619.3 Flat 5 Source 12 1
HOPS-71 4.9 277.5 I 2 -
HOPS-108 33.5 38.5 0 1 MIPS 2289 2
HOPS-368 60.2 137.5 I 1 Source 34 1
HOPS-369 30.9 379.2 Flat 1 Source 32 1
HOPS-370 315.7 71.5 I 1 VLA 11 2
HOPS-394 5.7 45.5 0 2 Source 9 1
HOPS-409 7.2 28.4 0 1 Source 43 1

Lbol, Tbol and Class from Furlan et al. (2016).

 

VLA Sources at centimetric wavelenghts.

Source Nature or Evolved Stage
Source 3 EG: Extragalactic
Source 4 HII: ionized region
Source 5 Disk Galaxy?
Source 6 ?
Source 7 Class I/II
Source 8 ?
Source 10 Class II
Source 12 Class I/II?
Source 13 EG: Extragalactic
Source 14 Class III
Source 15 ?
Source 16 ?
Source 17 Class III
Source 18 ?
Source 19 Class III
Source 20 Source 26 Knot?
Source 21 Class II/III
Source 22 Class III
Source 23 EG or Class II/III
Source 26 Radio Galaxy?
Source 27 Class III
Source 28 Class I/II
Source 29 Class I/II
Source 30 Source 26 knot?
Source 31 ?
Source 33 HII: ionized region
Source 35 EG or Class I/II
Source 36 Class III
Source 37 Class I/II
Source 38 YSO: Young Stellar Object
Source 40 Class III
Source 41 ?
Source 44 ?
Source 45 Class II/III
Source 47 Class III
MIPS 2301 YSO: Young Stellar Object
MIPS 2297 Class II
VLA 15 YSO: Young Stellar Object
VLA 16 YSO: Young Stellar Object

Data from Diaz-Rodriguez et al. (to be submitted) (1) except MIPS 2301, MIPS 2297, VLA 15 and VLA 16 from Osorio et al. (2017) (2) .