Free Access
Issue
A&A
Volume 552, April 2013
Article Number A122
Number of page(s) 19
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201118719
Published online 12 April 2013

Online material

Assignments of CH3OCH3, v = 0, v11 = 1, and v15 = 1 for G327.3-0.6 in all observed frequency windows

In this appendix we show the line parameters for all the unblended lines that have been detected for CH3OCH3, ν= 0 (Table A.1), ν11 = 1 (Table A.2), and ν15 = 1 (Table A.3). For questions about the full line-list please contact the authors. For all transitions frequencies, quantum numbers and the energies of the upper state (Eu) are given as well as the measured integrated line intensities () and model line-intensities from the isothermal myXCLASS model for the dimethyl ether emission (Imodel). Most features are actually composed of a set of multiple transitions, and we therefore refer to Endres et al. (2009) and Endres et al. (in prep.) for the values of μ2S for the individual transitions.

Table A.1

Detections of CH3OCH3, ν= 0 toward G327.3-0.6.

Table A.2

Detections of CH3OCH3, ν11 = 1, transitions found to be free of emission from other species toward G327.3-0.6.

Table A.3

Detections of CH3OCH3, ν15 = 1, found to be free of emission from other species toward G327.3-0.6.


© ESO, 2013

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