EDP Sciences
Herschel: the first science highlights
Free Access
Issue
A&A
Volume 518, July-August 2010
Herschel: the first science highlights
Article Number L83
Number of page(s) 6
Section Letters
DOI https://doi.org/10.1051/0004-6361/201014627
Published online 16 July 2010

Online Material

\begin{figure}
\par\includegraphics[width=90mm,clip]{14627fg5.eps}\includegraphics[width=88mm,clip]{14627fg6.eps}
\end{figure} Figure 5:

Left: extinction map of the RMC, derived from stellar reddening of background stars in JHK, using the 2MASS database, and a pixel size of $1.3\hbox {$^\prime $ }$ (Bontemps, priv. comm.; Schneider, et al. 2010). Contour levels increase from $A_{\rm V}=2^{\rm m}$ to $14^{\rm m}$ in steps of $2^{\rm m}$. Right: molecular hydrogen column density [cm-2] in logarithmic scaling determined from the same greybody fit that was used for the temperature. The regions referred to in Table 1 are indicated.

Open with DEXTER

\begin{figure}
\par\includegraphics[width=9cm,clip]{14627fg7.eps}\includegraphics[width=9cm,clip]{14627fg8.eps}
\end{figure} Figure 6:

Zoom into the Center ( left) and Monoceros Ridge ( right) regions, similar to the Extended Ridge presented in Fig. 4. Upper row: dust temperature, and column density plots of each region, respectively. Lower row: overlay 70 $\mu $m and 350 $\mu $m, and three-color image (70, 160, 250 $\mu $m) of each region, respectively.

Open with DEXTER

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