Herschel spectral surveys of star-forming regions - Overview of the 555–636 GHz range

Free Access

Issue		A&A Volume 521, October 2010 Herschel/HIFI: first science highlights


Article Number		L22
Number of page(s)		8
Section		Letters
DOI		https://doi.org/10.1051/0004-6361/201015081
Published online		01 October 2010

Online Material

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{15081fig2.ps} \end{figure}$	Figure 2: Zoom around the SO line 14₁₃-13₁₂ at 601.258 GHz. The other lines in the spectrum are from CH₃OH, CH₃OCH₃ as marked. Thre weaker lines are likely from ethanol (C₂H₅OH. Colours are as in Fig. 1. From bottom to top: L1157-B1, IRAS 16293-2422, OMC2-FIR4, AFGL 2591, and NGC 6334I.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{15081fig3.ps} \end{figure}$	Figure 3: Zoom around the HDO line 2_1,1-2_0,2 at 599.927 GHz and the H₂CO line 8_1,7-7_1,6 at 600.331 GHz. Colours are as in Fig. 1. From bottom to top: L1157-B1, IRAS 16293-2422, OMC2-FIR4, AFGL 2591, and NGC 6334I.
Open with DEXTER

$\begin{figure} \par\includegraphics[width=8.5cm,clip]{15081fig4.ps} \end{figure}$	Figure 4: Zoom around the CH₃OH lines of the 12-11 series. The transitions of the brightest lines are marked following the JPL catalog. The DNC 8-7 line lies at 579.205 GHz. Colours are as in Fig. 1. From bottom to top: L1157-B1, IRAS 16293-2422, OMC2-FIR4, AFGL 2591, and NGC 6334I.
Open with DEXTER

Table 3: List of detected lines, for all species except CH₃OH and CH₃OCH₃.

Table 4: List of detected lines of CH₃OH.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.