VLT-VIMOS integral field spectroscopy of luminous and ultraluminous infrared galaxies - II. Evidence for shock ionization caused by tidal forces in the extra-nuclear regions of interacting and merging LIRGs

Free Access

Issue		A&A Volume 517, July 2010


Article Number		A28
Number of page(s)		43
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/200913239
Published online		28 July 2010

Online Material

$\begin{figure} \par\includegraphics[width=14cm,clip]{13239fg14a.eps} \end{figure}$	Figure 14: Panel showing the images utilized for the morphological classification. The left column contains details about the size and scale for the displayed images, as well as relevant morphological features and final classification. The central and right columns display the Digital Sky Survey and HST images, respectively. Orientation is north up, east to the left.
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$\begin{figure} \par\includegraphics[width=14cm,clip]{13239fg14b.eps} \end{figure}$	Figure 14: continued.
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$\begin{figure} \par\includegraphics[width=14cm,clip]{13239fg14c.eps} \end{figure}$	Figure 14: continued.
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$\begin{figure} \par\includegraphics[width=14cm,clip]{13239fg14d.eps} \end{figure}$	Figure 14: continued.
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$\begin{figure} \par\includegraphics[width=14cm,clip]{13239fg14e.eps} \end{figure}$	Figure 14: continued.
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$\begin{figure} \par\includegraphics[width=14cm,clip]{13239fg14f.eps} \end{figure}$	Figure 14: continued.
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$\begin{figure} \par\includegraphics[width=14cm,clip]{13239fg14g.eps} \end{figure}$	Figure 14: continued.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg15a.ps} \end{figure}$	Figure 15: [S II] $\lambda \lambda$ 6717,6731/H $\alpha$ vs. [N II] $\lambda$ 6584/H $\alpha$ diagrams for the individual pointings.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg15b.ps} \end{figure}$	Figure 15: continued.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg16a.ps} \end{figure}$	Figure 16: [O I] $\lambda$ 6300/H $\alpha$ vs. [N II] $\lambda$ 6584/H $\alpha$ diagrams for the individual pointings.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg16b.ps} \end{figure}$	Figure 16: continued.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg17a.eps} \end{figure}$	Figure 17: Line ratios vs. velocity dispersions relation for the individual pointings.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg17b.eps} \end{figure}$	Figure 17: continued.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg17c.eps} \end{figure}$	Figure 17: continued.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg17d.eps} \end{figure}$	Figure 17: continued.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg17e.eps} \end{figure}$	Figure 17: continued.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg17f.eps} \end{figure}$	Figure 17: continued.
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$\begin{figure} \par\includegraphics[width=17cm,clip]{13239fg17g.eps} \end{figure}$	Figure 17: continued.
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