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IV. MPDG - Some preliminary results

Fabry-Perot interferometric study of ionized gas kinematics in XMD galaxies.

Fig. The results of Fabry-Perot interferometric study of XMD BCG HS 2236+1344 with two bright star-formation regions (probable merger). Upper row: Images in continuum and in H-alpha line in greyscale, with isophotes overlaid. Bottom row: the velocity field with the abrupt break, indicating the two components are probably unrelated (right); H-alpha line widths (FWHM) (or velocity dispersion) in km/s (also in greyscale and isolines) along the both components (left). Maximal values are observed on the border between the two components.

return 16 February 2008