| Issue |
A&A
Volume 573, January 2015
|
|
|---|---|---|
| Article Number | A73 | |
| Number of page(s) | 21 | |
| Section | Interstellar and circumstellar matter | |
| DOI | https://doi.org/10.1051/0004-6361/201424354 | |
| Published online | 22 December 2014 | |
Online material
Appendix A: Spectral fit figures
 |
Fig. A.1
Left: simultaneous spectral fits to the EPIC spectra of B1. Right: EPIC-pn spectrum of MCSNR J0536−6913 from Obs. ID 0601200101 (deepest EPIC-pn observation) with additive model components shown. The red dash-dot-dot-dot lines represent the AXB components, the magenta dash-dot line shows the instrumental fluorescence line, blue dotted lines mark the LMC ISM, and green dashed lines represent the source components (source model = vapec+pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
 |
Fig. A.2
As in Fig. A.1 for B2 (source model = pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
 |
Fig. A.3
As in Fig. A.1 for B3 (source model = pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
 |
Fig. A.4
As in Fig. A.1 for C1 (source model = pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
 |
Fig. A.5
As in Fig. A.1 for C2 (source model = pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
 |
Fig. A.6
As in Fig. A.1 for D (source model = pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
 |
Fig. A.7
As in Fig. A.1 for I1 (source model = vapec+pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
 |
Fig. A.8
As in Fig. A.1 for I2 (source model = pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
 |
Fig. A.9
As in Fig. A.1 for I3 (source model = pow). Best-fit parameters are given in Table 5. |
| Open with DEXTER | |
© ESO, 2014
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