| Title : (Tentative) 2D modelling the low surface brightness stellar host in BCDs : | ||||||
| Comparison with classical monodimentional ones | ||||||
| Authors : R.O. Amorin, J.A.L. Aguerri, C. Munoz-Tunon, L.M. Cairos | ||||||
| Abstract : | ||||||
| 2D Modelling the low surface brightness stellar host in BCDs: Comparison | ||||||
| with classical monodimensional ones. | ||||||
| In Blue Compact Dwarfs galaxies, the stellar and ionized gas emission from | ||||||
| the starburst overshines in the innermost part of the galaxy, | ||||||
| the low surface brightness (LSB) stellar component, so the study of this | ||||||
| stellar host relies enterely on the outer regions. | ||||||
| Here, as a part of a larger program, we fitted the LSB component with a | ||||||
| Sersic law using the 2D optical and NIR images after masking out the starburst with | ||||||
| the help of our H_alpha images and color maps. We compare | ||||||
| the sersic parameters determined with this method and previous fits of | ||||||
| averaged 1D profiles for two typical BCDs of our sample, Haro2 and Haro3. | ||||||