Kinetic temperatures toward X1/X2 orbit interceptions regions and giant molecular loops in the Galactic center region

D. Riquelme; M. A. Amo-Baladrón; J. Martín-Pintado; R. Mauersberger; S. Martín; L. Bronfman

doi:10.1051/0004-6361/201118288

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Volume 549 (January 2013)

A&A, 549 (2013) A36

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Issue		A&A Volume 549, January 2013


Article Number		A36
Number of page(s)		28
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201118288
Published online		13 December 2012

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Appendix A: Complementary tables

Table A.1

Fractional abundances of NH₃ with respect to SiO, HNCO, CS, C³⁴S, and of SiO and HNCO with respect to CS and C³⁴S.

Table A.2

Estimation of heating and cooling rates for each source.

Table A.3

Column density derived for NH3 (3, 3) and NH3 (6, 6) using RADEX.

Table A.4

Results from Gaussian fit and optical depth from NH₃ method.

Table A.5

Gaussian fits and column densities for SiO, C³⁴S, HNCO.

Appendix B: Complementary figures

This appendix presents the LVG diagrams of the metastable inversion transitions of para-NH₃. Most of the sources show two kinetic temperature components: one warm plotted in a red line; and one cool plotted in a blue line. In the cases where only the warm kinetic temperature component was present, the result is showed with a red line. We show the n(H₂) derived for each component from the CS data, which was used as a fixed parameter in the RADEX program. The shaded regions correspond to the error associated to each para-NH₃ line. When a line was not detected we plot their 3 − σ level with a dashed line. The error associated to the kinetic temperature and column density was estimated computing the χ² of the line intensities over the grid used for the LVG model. We impose , which translates in the 68.3% confidence level projected for each parameter axis, which is showed as a black elipse.

	Fig. B.1 LVG diagrams of NH₃ for each velocity component of Halo 1. Top: 87.7 km s^-1. Middle: 117.2 km s^-1. Bottom: 138.6 km s^-1.
Open with DEXTER

	Fig. B.2 LVG diagram of NH₃ for Halo 4.
Open with DEXTER

	Fig. B.3 LVG diagram of NH₃ for Disk X1-1. The blue lines correspond to the low-temperature regimen, and the red lines to the high-temperature regimen.
Open with DEXTER

	Fig. B.4 LVG diagram of NH₃ for Disk X2-1. The blue lines correspond to the low-temperature regimen, and the red lines to the high-temperature regimen.
Open with DEXTER

	Fig. B.5 LVG diagram of NH₃ for Disk X1-2. The blue lines correspond to the low-temperature regimen, and the red lines to the high-temperature regimen.
Open with DEXTER

	Fig. B.6 LVG diagram of NH₃ for Disk X2-2. The blue lines correspond to the low-temperature regimen, and the red lines to the high-temperature regimen.
Open with DEXTER

	Fig. B.7 LVG diagrams of NH₃ for each velocity component of Disk 1. Top: 56.5 km s^-1. Bottom: 72.4 km s^-1. The blue lines correspond to the low-temperature regimen, and the red lines to the high-temperature regimen.
Open with DEXTER

	Fig. B.8 LVG diagrams of NH₃ for each velocity component of Disk 2. Top: 48.8 km s^-1. Middle: 74.5 km s^-1. Bottom: 95.8 km s^-1. The blue lines correspond to the low-temperature regimen, and the red lines to the high-temperature regimen.
Open with DEXTER

	Fig. B.9 LVG diagrams of CS for each velocity component (defined by the J = 2−1 CS) of Halo 1 (see Table A.5). Top: 83.8 km s^-1. Middle: 117.4 km s^-1. Bottom: 136.9 km s^-1. The T_kin is indicated in the lower left corner in each plot.
Open with DEXTER

	Fig. B.10 LVG diagrams of CS for each velocity component of Halo 2. Top: −80 km s^-1. Bottom: −51.9 km s^-1.
Open with DEXTER

	Fig. B.11 LVG diagrams of CS for each velocity component of Halo 3. Top: −64.7 km s^-1. Bottom: −13.9 km s^-1.
Open with DEXTER

	Fig. B.12 LVG diagrams of CS for Halo 4.
Open with DEXTER

	Fig. B.13 LVG diagrams of CS for Halo 5.
Open with DEXTER

	Fig. B.14 LVG diagrams of CS for each kinetic temperature regime of Disk X1-1.
Open with DEXTER

	Fig. B.15 LVG diagrams of CS for each kinetic temperature regime of Disk X2-1.
Open with DEXTER

	Fig. B.16 LVG diagrams of CS for each kinetic temperature regime of Disk X1-2.
Open with DEXTER

	Fig. B.17 LVG diagrams of CS for each kinetic temperature regime of Disk X2-2.
Open with DEXTER

	Fig. B.18 LVG diagrams of CS for each kinetic temperature regime, for each velocity component of Disk 1. Top: 56.8 km s^-1. Bottom: 74.9 km s^-1.
Open with DEXTER

	Fig. B.19 LVG diagrams of CS for each kinetic temperature regime, for each velocity component of Disk 2. Top: 14.2 km s^-1. Middle: 55.9 km s^-1. Bottom: 79.0 km s^-1.
Open with DEXTER

© ESO, 2012

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