Astronomy & Astrophysics

All Figures

$\begin{figure} \par\rotatebox{-90}{ \includegraphics[height=13.8cm,width=14.8cm,clip]{H4129F1.ps} } \end{figure}$ Figure 1: The morphological make up of the parent sample (empty histograms) and the observed sample (filled histograms). See Sect. 3 for details.
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In the text

$\begin{figure} \par\rotatebox{-90}{ \includegraphics[height=14cm,width=15cm,clip]{H4129F2.ps} } \end{figure}$ Figure 2: The distribution of galaxy D₂₅ major-axis diameters in the parent sample (empty histograms) and the observed sample (filled histograms). See Sect. 3 for details.
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In the text

$\begin{figure} \par\rotatebox{-90}{ \includegraphics[height=14cm,width=15cm,clip]{H4129F3.ps} } \end{figure}$ Figure 3: The distribution of total R-band absolute magnitudes for the observed galaxies. See Sect. 3 for details.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F4.ps} \end{figure}$ Figure 4: Comparison of literature values for total galaxy H $\alpha +$ [N II] fluxes with values from the present study.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F5.ps} \end{figure}$ Figure 5: Comparison of literature values for total galaxy H $\alpha +$ [N II] EWs with values from the present study.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F6a.ps} \includ... ...ip]{H4129F6b.ps} \includegraphics[width=5.5cm,clip]{H4129F6c.ps} } \end{figure}$ Figure 6: UGC 859, SAB0/a (left); UGC 11238, SB0/a (centre); and UGC 12043, S0/a (right). For each galaxy, the top frame shows the H $\alpha +$ [N II] growth curve (circles), the R-band growth curve (asterisks) and the H $\alpha +$ [N II] EW (crosses) as a function of aperture size. The vertical scale relates to the EW plots, and is in nm; the H $\alpha +$ [N II] and R-band fluxes are normalised arbitrarily. The horizontal scale is the semi-major axis or radius of the apertures used, in units of 0 $.\!\!^{\prime\prime}$ 33 pixels. The images show the R-band (central frame) and continuum-subtracted H $\alpha +$ [N II] images (bottom frame), with superposed ellipses to show the apertures used for total line fluxes and R magnitudes.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F7a.ps} \includ... ...ip]{H4129F7b.ps} \includegraphics[width=5.5cm,clip]{H4129F7c.ps} } \end{figure}$ Figure 7: UGC 3685, SBb (left): UGC 4273, SBb (centre); and UGC 6077, SBb (right). See Fig. 6 for details.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F8a.ps} \includ... ...ip]{H4129F8b.ps} \includegraphics[width=5.5cm,clip]{H4129F8c.ps} } \end{figure}$ Figure 8: UGC 19, Sbc (left); UGC 6644, Sc (centre); and UGC 3711, IBm (right). See Fig. 6 for details.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F9a.ps} \includ... ...ip]{H4129F9b.ps} \includegraphics[width=5.5cm,clip]{H4129F9c.ps} } \end{figure}$ Figure 9: UGC 7326, Im (left); UGC 7866, IABm (centre); and UGC 8098, SBm (right). See Fig. 6 for details.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F10a.ps} \inclu... ...]{H4129F10b.ps} \includegraphics[width=5.5cm,clip]{H4129F10c.ps} } \end{figure}$ Figure 10: UGC 806, SABcd (left); UGC 3463, SABbc (centre); and UGC 5221, Sc (right). See Fig. 6 for details.
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In the text

$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F11a.ps} \inclu... ...]{H4129F11b.ps} \includegraphics[width=5.5cm,clip]{H4129F11c.ps} } \end{figure}$ Figure 11: UGC 12699, SBb pec (left); UGC 3847, Irr (centre); and UGC 5398, I0 (right). See Fig. 6 for details.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F12.ps} \end{figure}$ Figure 12: Distribution of star formation rates as a function of Hubble T type.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F13.ps} \end{figure}$ Figure 13: Mean and median star formation rates as a function of Hubble T type.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F14.ps} \end{figure}$ Figure 14: Mean star formation rates as a function of Hubble T type, separated into barred and unbarred types.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F15.ps} \end{figure}$ Figure 15: Distribution of H $\alpha +$ [N II] EWs as a function of Hubble T type.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F16.ps} \end{figure}$ Figure 16: Mean and median H $\alpha +$ [N II] EW as a function of Hubble T type.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F17.ps} \end{figure}$ Figure 17: Log H $\alpha +$ [N II] EW as a function of total R-band absolute magnitude. The dashed line shows the EW completeness limit of 0.4 nm.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F18.ps} \end{figure}$ Figure 18: H $\alpha +$ [N II] surface brightness as a function of galaxy type.
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In the text

$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F19.ps} \end{figure}$ Figure 19: H $\alpha +$ [N II] surface brightness as a function of total R-band absolute magnitude.
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In the text

$\begin{figure} \par\rotatebox{-90}{ \includegraphics[height=13.8cm,width=14.8cm,clip]{H4129F1.ps} } \end{figure}$	Figure 1: The morphological make up of the parent sample (empty histograms) and the observed sample (filled histograms). See Sect. 3 for details.
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$\begin{figure} \par\rotatebox{-90}{ \includegraphics[height=14cm,width=15cm,clip]{H4129F2.ps} } \end{figure}$	Figure 2: The distribution of galaxy D₂₅ major-axis diameters in the parent sample (empty histograms) and the observed sample (filled histograms). See Sect. 3 for details.
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$\begin{figure} \par\rotatebox{-90}{ \includegraphics[height=14cm,width=15cm,clip]{H4129F3.ps} } \end{figure}$	Figure 3: The distribution of total R-band absolute magnitudes for the observed galaxies. See Sect. 3 for details.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F4.ps} \end{figure}$	Figure 4: Comparison of literature values for total galaxy H $\alpha +$ [N II] fluxes with values from the present study.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F5.ps} \end{figure}$	Figure 5: Comparison of literature values for total galaxy H $\alpha +$ [N II] EWs with values from the present study.
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$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F7a.ps} \includ... ...ip]{H4129F7b.ps} \includegraphics[width=5.5cm,clip]{H4129F7c.ps} } \end{figure}$	Figure 7: UGC 3685, SBb (left): UGC 4273, SBb (centre); and UGC 6077, SBb (right). See Fig. 6 for details.
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$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F8a.ps} \includ... ...ip]{H4129F8b.ps} \includegraphics[width=5.5cm,clip]{H4129F8c.ps} } \end{figure}$	Figure 8: UGC 19, Sbc (left); UGC 6644, Sc (centre); and UGC 3711, IBm (right). See Fig. 6 for details.
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$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F9a.ps} \includ... ...ip]{H4129F9b.ps} \includegraphics[width=5.5cm,clip]{H4129F9c.ps} } \end{figure}$	Figure 9: UGC 7326, Im (left); UGC 7866, IABm (centre); and UGC 8098, SBm (right). See Fig. 6 for details.
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$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F10a.ps} \inclu... ...]{H4129F10b.ps} \includegraphics[width=5.5cm,clip]{H4129F10c.ps} } \end{figure}$	Figure 10: UGC 806, SABcd (left); UGC 3463, SABbc (centre); and UGC 5221, Sc (right). See Fig. 6 for details.
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$\begin{figure} \par\mbox{\includegraphics[width=5.5cm,clip]{H4129F11a.ps} \inclu... ...]{H4129F11b.ps} \includegraphics[width=5.5cm,clip]{H4129F11c.ps} } \end{figure}$	Figure 11: UGC 12699, SBb pec (left); UGC 3847, Irr (centre); and UGC 5398, I0 (right). See Fig. 6 for details.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F12.ps} \end{figure}$	Figure 12: Distribution of star formation rates as a function of Hubble T type.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F13.ps} \end{figure}$	Figure 13: Mean and median star formation rates as a function of Hubble T type.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F14.ps} \end{figure}$	Figure 14: Mean star formation rates as a function of Hubble T type, separated into barred and unbarred types.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F15.ps} \end{figure}$	Figure 15: Distribution of H $\alpha +$ [N II] EWs as a function of Hubble T type.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F16.ps} \end{figure}$	Figure 16: Mean and median H $\alpha +$ [N II] EW as a function of Hubble T type.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F17.ps} \end{figure}$	Figure 17: Log H $\alpha +$ [N II] EW as a function of total R-band absolute magnitude. The dashed line shows the EW completeness limit of 0.4 nm.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F18.ps} \end{figure}$	Figure 18: H $\alpha +$ [N II] surface brightness as a function of galaxy type.
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$\begin{figure} \par\includegraphics[angle=-90,width=10cm,clip]{H4129F19.ps} \end{figure}$	Figure 19: H $\alpha +$ [N II] surface brightness as a function of total R-band absolute magnitude.
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