A line confusion-limited millimeter survey of Orion KL - III. Sulfur oxide species

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Volume 556 (August 2013)

A&A, 556 (2013) A143

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Issue		A&A Volume 556, August 2013


Article Number		A143
Number of page(s)		50
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201321285
Published online		09 August 2013

Online material

Appendix A: Figures and tables

Table A.1

SO emission line parameters obtained from Gaussian fits.

Table A.2

SO₂ parameters from Gaussian fits (lines at 1.3 mm).

Table A.3

SO₂ parameters from Gaussian fits (lines at 2−3 mm).

Table A.4

Rotational temperatures, T_rot, and column densities, N, obtained from rotational diagrams.

Table A.5

Isotopologue ratios and molecular ratios.

Table A.6

Molecular abundances, X.

Table A.7

Column density upper limits for undetected sulfur-bearing molecules in Orion KL.

	Fig. A.1 Rotational diagrams for the plateau, high-velocity plateau, and hot core components. Black dots for SO₂ and green dots for SO. The black and green lines are the best linear fits to the SO₂ and SO points, respectively.
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	Fig. A.2 Rotational diagrams for the compact ridge, extended ridge, and 20.5 km s^-1 component. Black dots for SO₂ and green dots for SO. The black and green lines are the best linear fits to the SO₂ and SO points, respectively.
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	Fig. A.3 Observed lines of ³³SO (black histogram) and best fit LVG model results (red).
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	Fig. A.4 Observed lines of S¹⁸O (black histogram) and best fit LVG model results (red).
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	Fig. A.5 Observed lines of ³³SO₂ (black histogram) and best fit LTE model (red). Boxes in black, blue, and green correspond to frequencies at 1.3, 2, and 3 mm, respectively.
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	Fig. A.6 Observed lines of SO¹⁸O (black histogram) and best fit LTE model (red).
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	Fig. A.7 Observed lines of SO¹⁷O (black histogram) and best fit LTE model (red).
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	Fig. A.8 Observed lines of ³⁴SO₂ν₂ = 1 (black histogram) and best fit LTE model (red).
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Table A.8

Observed lines of SO and its isotopologues.

Table A.9

Observed lines of SO₂, its isotopologues, and vibrationally excited states.

© ESO, 2013

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