| Issue |
A&A
Volume 561, January 2014
|
|
|---|---|---|
| Article Number | A50 | |
| Number of page(s) | 20 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201322150 | |
| Published online | 23 December 2013 | |
Online material
Appendix A
Appendix A.1: PACS spatial pixel emissions
 |
Fig. A.1
[O i] 63 μm spectrum for each pixel in the PACS spectrometer array. The PACS integral filed unit has a 47′′ × 47′′ field of view. Each 25 pixels has a 9.4′′ × 9.4′′ spatial resolution. The flux is emitted in the central spaxels. |
| Open with DEXTER | |
 |
Fig. A.2
[O i] 145 μm spectrum for each pixel in the PACS spectrometer array. |
| Open with DEXTER | |
 |
Fig. A.3
[C ii] spectrum for each pixel in the PACS spectrometer array. The [C ii] 157μm line is detected in the central spaxel. |
| Open with DEXTER | |
Appendix A.2: Collisional data
The original articles for the line frequencies, Einstein coefficients, and collisional rates are CO (Flower 2001; Jankowski & Szalewicz 2005; Yang et al. 2006; Wernli et al. 2006), H2O (Barber et al. 2006; Dubernet & Grosjean 2002; Faure et al. 2004, 2007; Daniel et al. 2011), O i (Abrahamsson et al. 2007; Bell et al. 1998; Chambaud et al. 1980; Jaquet et al. 1992; Launay & Roueff 1977), C ii (Flower & Launay 1977; Launay & Roueff 1977; Wilson & Bell 2002), CH+ (Müller 2010; Lim et al. 1999; Hammami et al. 2009; Turpin et al. 2010), OH (Offer et al. 1994).
Appendix A.3: Photometric data
We provide the photometric data used in our SED modeling in Table A.1.
Non-simultaneous photometric data.
© ESO, 2013
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