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Дата изменения: Sat Feb 16 19:38:31 2008 Дата индексирования: Tue Oct 2 02:51:39 2012 Кодировка: Поисковые слова: http astrokuban.info astrokuban |
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.