next previous
Up: The 1 to 2.5  Galaxies


Online Material


 \begin{figure}\par\includegraphics[width=12cm]{haro14ir.eps}
\end{figure} Figure 1: K band contour plots and light profiles of the observed BCDGs. The outermost isophote corresponds to a signal-to-noise ratio of 1.75 (approx. 22 mag arcsec-2), and spaced by 1 in units of S/N. The bar at the bottom of the contour plots represents 1 Kpc assuming H0 = 80 km s-1. The color profiles (J-H, H-J and J-K) are displayed in individual graph for clarity. The bottom three graph show the J, H, K band light profiles as functions of the equivalent radius (in arcsec), the logarithm radius and the reduced r1/4 radius. This Figure is only available in electronic form at http://www.edpsciences.org


 \begin{figure}\par\includegraphics[width=13cm]{mk996ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{mk600ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{fair301ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{tol0610ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{tol0645ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{tol0954ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{tol0957ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{tol3ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{um465ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{comp465ir.eps}
\end{figure} Figure 1: continued


 \begin{figure}\par\includegraphics[width=13cm]{um461ir.eps}
\end{figure} Figure 1: continued


next previous
Up: The 1 to 2.5  Galaxies

Copyright ESO 2001