Issue
A&A
Volume 518, July-August 2010
Herschel: the first science highlights
Article Number L149
Number of page(s) 6
Section Letters
DOI https://doi.org/10.1051/0004-6361/201014655
Published online 16 July 2010

Online Material

\begin{figure}
\par\includegraphics[angle=270,width=13.3cm,clip]{14655fg2.ps}\vspace*{7mm}
\end{figure} Figure 2:

Spectra of C/2006 W3 (Christensen) obtained with PACS on November 8, 2009 (central pixel pointed on the comet nucleus). The pixel size is $9.4\hbox {$^{\prime \prime }$ }\times 9.4\hbox {$^{\prime \prime }$ }$. The wavelengths of water lines are indicated by vertical dashed lines.

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\begin{figure}
\par\includegraphics[width=7.5cm,clip]{14655fg5.ps}
\end{figure} Figure 5:

Spectra of C/2006 W3 (Christensen) observed with the IRAM 30-m telescope.

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\begin{figure}
\par\includegraphics[width=8cm,clip]{14655fg6.ps}
\end{figure} Figure 6:

Comparison of measured abundances relative to HCN in comets C/2006 W3 (Christensen) and C/1995 O1 (Hale-Bopp) at 3.3 AU from the Sun.

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