Issue |
A&A
Volume 567, July 2014
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Article Number | A108 | |
Number of page(s) | 21 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201423440 | |
Published online | 22 July 2014 |
Online material
Appendix A
Fig. A.1
Color−coded SOFI image of F19 obtained in on-off mode. The J , H , and Ks bands are coded in blue, green, and red. |
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Open with DEXTER |
Fig. A.2
Color−coded SOFI image of F19 obtained in jitter mode. The Js, H , and Ks bands are coded in blue, green, and red. |
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Fig. A.3
Jittered JsHKs (left) and on-off JHKs (right) image of F8. |
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Fig. A.4
NB 2.124 H2 S(1) image of fields 7, 8, 14, and 15. |
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Fig. A.5
NB 2.090 continuum image of fields 7, 8, 14, and 15. |
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Fig. A.6
NB 1.257 continuum image of F15. |
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Fig. A.7
NB 2.167 Brγ image of F14. |
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Fig. A.8
The J−H, H−Ks color−color diagram of the shell (left panel) and background (right panel) objects in F7. Filled circles mark the observed stars and boxes mark the stars behind the globulettes. Asterisks mark stars with only H−Ks colors. The crosses in the bottom righthand corner indicate the maximum (left) and the average error (right). A reddening vector of 3m is indicated. |
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Fig. A.9
As Fig. A.8 of F8. |
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Fig. A.10
As Fig. A.8 of F15. F15-tip is at the northern edge of frame F15. |
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Fig. A.11
The J−H, H−Ks color−color diagram of all objects in F19. Markings are as in Fig. A.8. There is no continuous shell detected in F19, so all stars are counted as background stars and plotted in the same diagram. 129-tail marks a star seen in the more diffuse part of the tail in RN 129 and has been marked for visual reference. |
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Fig. A.12
PACS 70 μm negative image covering fields 8, 14, 15, and 19. |
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Fig. A.13
PACS 160 μm negative image covering fields 8, 14, 15, and 19. |
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© ESO, 2014
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