Hα surface photometry of galaxies in the Virgo cluster -: III.: Observations with INT and NOT 2.5 m telescopes

We present Halpha line imaging observations of 30 galaxies obtained at the 2.5 m INT and NOT telescopes. The observed galaxies are mostly BCD Virgo cluster galaxies. Halpha+[NII] fluxes and equivalent widths, as well as images of all the detected targets are presented. With these observations, Halpha data are available for similar or equal to50% of the BCD galaxies listed in the VCC.