Deuteration around the ultracompact HII region Monoceros R2

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Volume 569 (September 2014)

A&A, 569 (2014) A19

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Issue		A&A Volume 569, September 2014


Article Number		A19
Number of page(s)		30
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201423407
Published online		10 September 2014

Online material

Appendix A: Tables and figures

In this section we show all the spectra of the hydrogenated (Figs. A.1–A.8) and deuterated (Figs. A.9–A.12) species toward the IF and MP2 positions. The tables of the parameters (Table A.1), the tables of the Gaussian fits (Tables A.2 –A.4), and the molecular abundances of HCN, HCO⁺, and C₂ relative to H₂ predicted by models A to D (Fig. A.13).

Table A.1

Observational parameters.

Table A.2

Gaussian fit parameters of the deuterated molecules at the IF and MP2 positions.

Table A.3

Gaussian fit parameters of the hydrogenated molecules at the IF position.

Table A.4

Gaussian fit parameters of the hydrogenated molecules at the MP2 position.

	Fig. A.1 C₂H spectra at the IF and MP2 positions. The red dashed lines mark different C₂H transitions. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequencies 87.317, 87.401, 262.004, and 262.064 GHz, from top to bottom.
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Fig. A.2

Panels 1 and 2: HCN spectra at the IF and MP2 positions. The red dashed lines mark different HCN transitions.The blue dashed line shows the velocity of 10 km s^-1, relative to the rest frequency of the transitions, 88.631 and 265.88 GHz. Panels 3 and 4: H¹³CN spectra at the IF and MP2 positions, the red dashed lines mark different H¹³CN transitions. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequencies 86.340 (panel 3) and 259.054 GHz (panel 4).

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	Fig. A.3 Panels 1 and 2: HC¹⁵N spectra at the IF and MP2 positions. The blue dashed line shows the velocity of 10 km s^-1 relative to 86.054, and 258.156 GHz, for panels 1 and 2, respectively. Panels 3 and 4: HN¹³C spectra at the IF and MP2 positions at 87.090, and 261.263 GHz.
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	Fig. A.4 Panels 1 and 2: H¹⁵NC spectra at the IF and MP2 positions. Panels 3 and 4: HNC spectra at the IF and MP2 poitions. The blue dashed line shows the velocity of 10 km s^-1 relative to 88.865, 266.587, 90.663, and 271.981 GHz, respectively.
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	Fig. A.5 H₂CO spectra at the two positions IF and MP2. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequencies 145.602, 211.211, 218.222, and 218.697 GHz, from top to bottom.
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	Fig. A.6 Panels 1 and 2: HC¹⁸O⁺ spectra at the two positions IF and MP2. Panels 3 and 4: H¹³CO⁺ spectra at the two positions IF and MP2. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequencies 85.162, 255.480, 86.745, and 260.255 GHz, from top to bottom.
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Fig. A.7

Panels 1 and 2 are the HCO spectra at the two positions IF and MP2. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequency 96.375 GHz, in panel 1, and 141.983 GHz, in panel 2. Panels 3 and 4 show the HCO⁺ spectra toward the two positions IF and MP2. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequency 89.188 GHz, in panel 3, and 267.557 GHz, in panel 4.

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	Fig. A.8 N₂H⁺ spectra at 93.173 GHz at the two positions IF and MP2. The red dashed lines mark different transitions of this molecule. The blue dashed line shows the velocity of 10 km s^-1 relative to the frequency of 93.137 GHz.
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	Fig. A.9 C₂D spectra at the two positions IF and MP2. The red dashed lines mark different C₂D transitions. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequencies 144.241, 144.297, 216.373, and 216.428 GHz, from top to bottom.
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	Fig. A.10 DCN and DNC spectra at the two positions IF and MP2. The red dashed lines mark different transitions. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequencies 144.828, 217.238 (for DCN), 152.609, and 228.91 GHz (for DNC), from top to bottom.
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Fig. A.11

Panels 1 and 2: DCO⁺ spectra at the two positions IF and MP2. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequencies 144.077 (in the top panel) and 216.112 GHz (in the bottom panel). Panel 3: D₂CO spectra at the two positions IF and MP2. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequency 110.837 GHz. Panel 4: N₂D⁺ spectra at the two positions IF and MP2. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequency 154.217 GHz.

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	Fig. A.12 Panels 1 to 3: HDCO spectra at the two positions IF and MP2. The blue dashed line shows the velocity of 10 km s^-1, relative to the frequencies 134.284, 257.748, and 268.290 GHz. Panel 4: NH2D spectra at IF and MP2 poitions, the blue dashed line shows the velocity of 10 km s^-1, relative to 85.925 GHz.
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Fig. A.13

Molecular abundances relative to H₂ predicted by models A to D. The input parameters of these models are shown in Table 4. The red line represents the [HCN]/[H₂] ratio, the purple line shows the [HCO⁺]/[H₂] ratio, and the blue line shows the [C₂H]/[H₂] ratio. The dashed lines shows the ratios of observational results toward MonR2 for the 10.5 km s^-1 component at the IF position.

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© ESO, 2014

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