| 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}](/articles/aa/olm/2010/10/aa14655-10/img105.png){kind=small}
|
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
|
| Open with DEXTER | |
.
The wavelengths of
water lines are indicated by vertical dashed lines.
![\begin{figure}
\par\includegraphics[width=7.5cm,clip]{14655fg5.ps}
\end{figure}](/articles/aa/olm/2010/10/aa14655-10/img106.png)
|
Figure 5: Spectra of C/2006 W3 (Christensen) observed with the IRAM 30-m telescope. |
| Open with DEXTER | |
![\begin{figure}
\par\includegraphics[width=8cm,clip]{14655fg6.ps}
\end{figure}](/articles/aa/olm/2010/10/aa14655-10/img107.png)
|
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. |
| Open with DEXTER | |
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