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Table 2

Orion-KL molecular components.

Component RAJ2000 DecJ2000 Size νLSR Δv TKin n(H2) N(H2)
05h35m... 05°22... (arcsec) (km s-1) (km s-1) (K) (cm-3) (cm-2)

extended ridge 146 21.̋5 ~180 8–10 2.5–5 40–60 ~1 × 105 7.1 × 1022
plateau 14516 30.̋59 20–30 5–10 20 95–150 1–10 × 106 1.8 × 1023
hot core 146 31.̋0 5–10 4–6 5–15 150–400 1–10 × 107 3.1–10 × 1023
hot core (peak) 7.3 × 108 5.4 × 1024
compact ridge/MF1 1409 36.̋9 5–15 7–9 1–2 80–150 1–10 × 106 3.9 × 1023
compact ridge (peak) 6.8 × 108 5.0 × 1024
IRc7 1426 31.̋29 ~2 2– 8 2.5–5 ~160
IRc21 14557 27.̋13 ~2 ~6 2.5 ~160
MF2 1444 34.̋4 ~2 3–17 2.5–6 100–150 4.2 × 108 3.1 × 1024
MF4/IRc20 14132 29.̋3 ~2 7–14 2–8 ~100 2.2 × 108 1.6 × 1024
MF5/IRc6 14158 27.̋83 ~2 6.5–13 2.5–6 ~100 2.2 × 108 1.6 × 1024
MF10/IRc2 1463 28.̋9 ~2 -3–7 3–5 150–200
MF12/IRc4 14188 34.̋44 ~2 0–11 2–5 100–150
EGP 1447 33.̋17 ~2 7–12 3–6 100–140

Notes. For further details see Irvine et al. (1987), Blake et al. (1987), and Favre et al. (2011a). Extended Ridge and Plateau are quoted for completeness but not discussed in this paper, their positions are simply given as those of Orion KL and Source I, respectively. All other source positions and sizes are from this paper or from Favre et al. (2011a) except EGP = ethylene glycol peak from Brouillet et al. (2015). Peak densities and column densities for the HC and the CR and for some of the MF peaks are measured in a 1.8′′ × 0.8′′ beam (Favre et al. 2011a) but should be considered cautiously. Our positions of IRc7 and IRc21 are closer to the positions of C23 and C13 sources of Friedel & Weaver (2011) than to the IRc positions of Shuping et al. (2004) while they are probably the same objects, respectively.

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