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| The last update of data | 2016-04-10 | Visitors: | 96943 | Questions and comments: | lvg@sao.ru |
Publications
Figure 1. The ratio of Hα-to-FUV star formation rates as a function of different global galaxy parameters
Figure 2. The ratio of Hα-to-FUV SFRs vs. apparent axial ratio for spiral galaxies and late-type irregular dwarfs
Figure 3. The ratio of Hα-to-FUV SFRs vs. morphological type of galaxies and vs. the mean B-band surface brightness
Figure 4. Specific star formation rates of nearby galaxies vs. their different global parameters
Figure 5. Integral SFR vs. total hydrogen mass for the Local Volume galaxies.
Figure 6. Specific star formation rate of nearby galaxies vs. their blue surface brightness
Figure 7. Specific star formation rate for the dwarf (log M* < 9) Local Volume galaxies as a function of two environment parameters
Figure 8. The diagnostic "past-future" diagram for the early-type galaxies, spiral galaxies and late-type dwarfs