Deep Near Infrared Mapping of Young and Old Stars in Blue Compact Dwarf Galaxies

Details Deep Near Infrared Mapping of Young and Old Stars in Blue Compact Dwarf Galaxies Deep Near Infrared Mapping of Young and Old Stars in Blue Compact Dwarf Galaxies

2003-06-16

arxiv.org/abs/astro-ph/0306307v1

Astrophys.J. 593 (2003) 312

Astronomy and Astrophysics

Astrophysics

49 pages, 9 figures, 10 tables, accepted for publication in the Astrophysical Journal

Scientific paper

10.1086/376516

We analyze J, H and Ks near-infrared data for 9 Blue Compact Dwarf (BCD) galaxies, selected from a larger sample that we have already studied in the optical. We present contour maps, surface brightness and color profiles, as well as color maps of the sample galaxies. The morphology of the BCDs in the NIR has been found to be basically the same as in the optical. The inner regions of these systems are dominated by the starburst component. At low surface brightness levels the emission is due to the underlying host galaxy; the latter is characterized by red, radially constant colors and isophotes well fit by ellipses. We derive accurate optical near--infrared host galaxy colors for eight of the sample galaxies; these colors are typical of an evolved stellar population. Interestingly, optical near--infrared color maps reveal the presence of a complex, large-scale absorption pattern in three of the sample galaxies. We study the applicability of the Sersic law to describe the surface brightness profiles of the underlying host galaxy, and find that, because of the limited surface brightness interval over which the fit can be made, the derived Sersic parameters are very sensitive to the selected radial interval and to errors in the sky subtraction. Fitting an exponential model gives generally more stable results, and can provide a useful tool to quantify the structural properties of the host galaxy and compare them with those of other dwarf classes as well as with those of star-forming dwarfs at higher redshifts.

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