Hα3: an Hα imaging survey of HI selected galaxies from ALFALFA III. Nurture builds up the Hubble sequence in the Great Wall

Context. We present the analysis of H alpha 3, an H alpha narrow band imaging follow up survey of galaxies selected from the HI Arecibo Legacy Fast ALFA Survey (ALFALFA) in the Coma supercluster. Aims. Taking advantage of H alpha 3, which provides the complete census of the recent star formation in HI rich galaxies in the local universe, we explored the hypothesis that a morphological sequence of galaxies of progressively earlier type and lower gas content exists in the neighborhood of a rich cluster of galaxies such as Coma, with a specific star formation activity that decreases with increasing local galaxy density and velocity dispersion. Methods. By using the H alpha hydrogen recombination line as a tracer of the instantaneous star formation, complemented with optical colors from SDSS, we investigated the relationships between atomic neutral gas and newly formed stars in different local galaxy density intervals, for many morphological types, and over a wide range of stellar masses (10(9) to 10(11.5) M-circle dot). Results. In the dwarf regime (8.5 < log (M-*/M-circle dot) < 9.5) we identify a four step sequence of galaxies with progressively redder colors (corrected for dust extinction), i.e., of decreasing specific star formation, from (1) HI rich late type galaxies (LTGs) belonging to the blue cloud that exhibit extended plus nuclear star formation, (2) similar to 0.1 mag redder, HI poor LTGs with nuclear star formation only, (3) similar to 0.35 mag redder, HI poor galaxies without either extended or nuclear star formation, but with nuclear post star burst (PSB) signature, (4) similar to 0.5 mag redder early type galaxies (ETGs) that belong to the red sequence, and show no gas or star formation on all scales. Along this sequence the quenching of the star formation proceeds radially outside in. The progression toward redder colors found along this morphological (gas content) sequence is comparable to the one obtained from increasing the local galaxy density, from cosmic filaments (1 2), to the rich clusters (2 3 4). Conclusions. In the dwarf regime we find evidence for an evolution of HI rich LTGs into ETGs through HI poor LTGs and PSB galaxies driven by the environment. We identify ram pressure as the mechanism most likely responsible for this transformation. We conclude that infall of galaxies has proceeded for the last 7.5 Gyr, building up the Coma cluster at a rate of approximately 100 galaxies with log (M-*/M-circle dot) > 9.0 per Gyr.