| 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.
Detections of CH3OCH3, ν= 0 toward G327.3-0.6.
Detections of CH3OCH3, ν11 = 1, transitions found to be free of emission from other species toward G327.3-0.6.
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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