EDP Sciences
Free Access
Issue
A&A
Volume 503, Number 3, September I 2009
Page(s) 801 - 816
Section Galactic structure, stellar clusters, and populations
DOI https://doi.org/10.1051/0004-6361/20079145
Published online 15 June 2009

Online Material

Appendix A: K$_{\rm s}$ images for all observed fields

This appendix contains the $K_{\rm s}$ images for all observed fields; these are also available at http://galatea.ifsi-roma.inaf.it/faustini/K-images/

 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m003.ps} }
\end{figure} Figure A.1:

$K_{\rm s}$ image of field Mol003 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m008.ps} }
\end{figure} Figure A.2:

$K_{\rm s}$ image of field Mol008 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m009.ps} }
\end{figure} Figure A.3:

$K_{\rm s}$ image of field Mol009; no submillimeter image is available for this field.

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m011.ps} }
\end{figure} Figure A.4:

$K_{\rm s}$ image of field Mol011 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m012.ps} }
\end{figure} Figure A.5:

$K_{\rm s}$ image of field Mol012 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m015.ps} }
\end{figure} Figure A.6:

$K_{\rm s}$ image of field Mol015; no submillimeter image is available for this field.

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m028.ps} }
\end{figure} Figure A.7:

$K_{\rm s}$ image of field Mol028; no submillimeter image is available for this field.

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m030.ps} }
\end{figure} Figure A.8:

$K_{\rm s}$ image of field Mol030; no submillimeter image is available for this field. The white cross marks the position of the IRAS source.

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m038.ps} }
\end{figure} Figure A.9:

$K_{\rm s}$ image of field Mol038 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m045.ps} }
\end{figure} Figure A.10:

$K_{\rm s}$ image of field Mol045 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m050.ps} }
\end{figure} Figure A.11:

$K_{\rm s}$ image of field Mol050; no submillimeter image is available for this field. The white cross marks the position of the IRAS source.

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m059.ps} }
\end{figure} Figure A.12:

$K_{\rm s}$ image of field Mol059 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m075.ps} }
\end{figure} Figure A.13:

$K_{\rm s}$ image of field Mol075 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m082.ps} }
\end{figure} Figure A.14:

$K_{\rm s}$ image of field Mol082; no submillimeter image is available for this field. The white cross marks the position of the IRAS source.

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m084.ps} }
\end{figure} Figure A.15:

$K_{\rm s}$ image of field Mol084; no submillimeter image is available for this field. The white cross marks the position of the IRAS source.

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m098.ps} }
\end{figure} Figure A.16:

$K_{\rm s}$ image of field Mol098 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m099.ps} }
\end{figure} Figure A.17:

$K_{\rm s}$ image of field Mol099; no submillimeter image is available for this field. The white cross marks the position of the IRAS source.

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m103.ps} }
\end{figure} Figure A.18:

$K_{\rm s}$ image of field Mol103 with superimposed SIMBA 1.2mm continuum in white contours ( Beltrán et al. 2006).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m109.ps} }
\end{figure} Figure A.19:

$K_{\rm s}$ image of field Mol109 with superimposed SIMBA 1.2mm continuum in white contours ( Beltrán et al. 2006).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m110.ps} }
\end{figure} Figure A.20:

$K_{\rm s}$ image of field Mol110 with superimposed SIMBA 1.2mm continuum in white contours ( Beltrán et al. 2006).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m136.ps} }
\end{figure} Figure A.21:

$K_{\rm s}$ image of field Mol136 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

Open with DEXTER

 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m139.ps} }
\end{figure} Figure A.22:

$K_{\rm s}$ image of field Mol139 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m143.ps} }
\end{figure} Figure A.23:

$K_{\rm s}$ image of field Mol143 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

Open with DEXTER

 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m148.ps} }
\end{figure} Figure A.24:

$K_{\rm s}$ image of field Mol148 with superimposed MAMBO 1.1 mm continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m151.ps} }
\end{figure} Figure A.25:

$K_{\rm s}$ image of field Mol151 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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 \begin{figure}
\par {\includegraphics[angle=-90,width=13cm,clip]{map_m160.ps} }
\end{figure} Figure A.26:

$K_{\rm s}$ image of field Mol160 with superimposed SCUBA 850 $\mu $m continuum in white contours (Molinari et al. 2008a).

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Appendix B: $K_{\rm s}$ luminosity functions

This appendix presents the set of background-subtracted $K_{\rm s}$ luminosity functions for all detected clusters. Material can also be retrieved at http://galatea.ifsi-roma.inaf.it/faustini/KLF/

\begin{figure}
\par\resizebox{18cm}{!}
{\includegraphics[angle=-0,origin=c,width...
...ps}
\includegraphics[angle=-0,origin=c,width=6cm]{KLF_mol008B.ps}}
\end{figure} Figure B.1:

Mol003 ( left), Mol008A ( center), Mol008B ( right).

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\begin{figure}
\par\resizebox{18cm}{!}
{\includegraphics[angle=-0,origin=c,width...
....ps}
\includegraphics[angle=-0,origin=c,width=6cm]{KLF_mol012.ps}}
\end{figure} Figure B.2:

Mol009 ( left), Mol011 ( center), Mol012 ( right).

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\begin{figure}
\par\resizebox{18cm}{!}
{\includegraphics[angle=-0,origin=c,width...
....ps}
\includegraphics[angle=-0,origin=c,width=6cm]{KLF_mol045.ps}}
\end{figure} Figure B.3:

Mol015 ( left), Mol028 ( center), Mol045 ( right).

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\begin{figure}
\par\resizebox{18cm}{!}
{\includegraphics[angle=-0,origin=c,width...
....ps}
\includegraphics[angle=-0,origin=c,width=6cm]{KLF_mol082.ps}}
\end{figure} Figure B.4:

Mol050 ( left), Mol075 ( center), Mol082 ( right).

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\begin{figure}
\par\resizebox{18cm}{!}
{\includegraphics[angle=-0,origin=c,width...
....ps}
\includegraphics[angle=-0,origin=c,width=6cm]{KLF_mol103.ps}}
\end{figure} Figure B.5:

Mol084 ( left), Mol099 ( center), Mol103 ( right).

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\begin{figure}
\par\resizebox{18cm}{!}
{\includegraphics[angle=-0,origin=c,width...
....ps}
\includegraphics[angle=-0,origin=c,width=6cm]{KLF_mol136.ps}}
\end{figure} Figure B.6:

Mol136 ( left), Mol110 ( center), Mol136 ( right).

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\begin{figure}
\par\resizebox{18cm}{!}
{\includegraphics[angle=-0,origin=c,width...
....ps}
\includegraphics[angle=-0,origin=c,width=6cm]{KLF_mol148.ps}}
\end{figure} Figure B.7:

Mol139 ( left), Mol143 ( center), Mol148 ( right).

Open with DEXTER

\begin{figure}
\par\resizebox{18cm}{!}
{\includegraphics[angle=-0,origin=c,width...
....ps}
\includegraphics[angle=-0,origin=c,width=6cm]{KLF_mol160.ps}}
\end{figure} Figure B.8:

Mol151 ( left), Mol160 ( right).

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