The host in blue compact galaxies. - Structural properties and scaling relations

R. Amorín; J. A. L. Aguerri; C. Muñoz-Tuñón; L. M. Cairós

doi:10.1051/0004-6361/200809591

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Volume 501 / No 1 (July I 2009)

A&A, 501 1 (2009) 75-88

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Issue		A&A Volume 501, Number 1, July I 2009


Page(s)		75 - 88
Section		Extragalactic astronomy
DOI		https://doi.org/10.1051/0004-6361/200809591
Published online		05 May 2009

Online Material

Table 4: Parameters for the underlying stellar host derived from the 2D Sérsic fit.

$\begin{figure}\par\includegraphics[width=17.5cm,angle=0]{9591f14a.eps}\\ [7pt] ... ...7pt] \includegraphics[width=17.5cm,angle=0]{9591f14e.eps}\\ [7pt]\end{figure}$

Figure 10:

Atlas of galaxy images I: Galaxies with Q=1. Broad-band galaxy images ( left), the best 2D Sérsic model ( centre) and the residual image ( right) of the 20 galaxies fitted with quality index Q=1 in the full sample of 28 BCGs. Broad-band images and 2D Sérsic models are showed in surface brightness grey scale (magnitude per square arcseconds). Realistic Poissonian noise are included in the 2D models. Residual images, i.e. galaxy-model, are displayed in an inverted linear grey scale (counts) which covers the range $\pm$ $3\sigma$ , where $\sigma$ is the mean rms of the sky background. Thus, darkest regions are the most luminous regions (mainly the starburst) which have been saturated to enhance residual features in the outer fitted regions, e.g. the host galaxy region. In all cases, horizontal and vertical axis are in pixels whereas the orientation is north (up) - east ( left).

Open with DEXTER

$\begin{figure}\includegraphics[width=17.5cm,angle=0]{9591f14f.eps}\\ [7pt] \inc... ...7pt] \includegraphics[width=17.5cm,angle=0]{9591f14i.eps}\\ [7pt]\end{figure}$	Figure 10: continued.
Open with DEXTER

$\begin{figure}\includegraphics[width=17.5cm,angle=0]{9591f14j.eps}\\ [7pt] \inc... ...pt] \includegraphics[width=17.5cm,angle=0]{9591f14m.eps}\\ [7pt]\end{figure}$	Figure 10: continued.
Open with DEXTER

$\begin{figure}\includegraphics[width=17.5cm,angle=0]{9591f14b.eps}\\ [7pt] \inc... ...pt] \includegraphics[width=17.5cm,angle=0]{9591f14p.eps}\\ [7pt]\end{figure}$	Figure 10: continued.
Open with DEXTER

$\begin{figure}\includegraphics[width=17.5cm,angle=0]{9591f14q.eps}\\ [7pt] \inc... ...pt] \includegraphics[width=17.5cm,angle=0]{9591f14t.eps}\\ [7pt]\end{figure}$	Figure 10: continued.
Open with DEXTER

$\begin{figure}\includegraphics[width=17.5cm,angle=0]{9591f15a.eps}\\ [7pt] \inc... ...pt] \includegraphics[width=17.5cm,angle=0]{9591f15d.eps}\\ [7pt]\end{figure}$	Figure 11: Atlas of galaxy images II: Galaxies with Q=2. Broad-band galaxy images ( left), the best 2D Sérsic model ( centre) and the residual image ( right) of the 8 galaxies fitted with quality index Q=2 in the full sample of 28 BCGs. The description is the same as in Fig. 10.
Open with DEXTER

$\begin{figure}\includegraphics[width=17.5cm,angle=0]{9591f15e.eps}\\ [7pt] \inc... ...pt] \includegraphics[width=17.5cm,angle=0]{9591f15h.eps}\\ [7pt]\end{figure}$	Figure 11: continued.
Open with DEXTER

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