Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. V: The Coma Supercluster survey completion

@article{Gavazzi2015Halpha3AH,
  title={Halpha3: an Halpha imaging survey of HI selected galaxies from ALFALFA. V: The Coma Supercluster survey completion},
  author={Giuseppe Gavazzi and Guido Consolandi and E. Viscardi and Matteo Fossati and Giulia A. D. Savorgnan and Michele Fumagalli and Leonel Guti{\'e}rrez and Hector Hernandez Toledo and Alessandro Boselli and Riccardo Giovanelli and Martha P. Haynes},
  journal={arXiv: Astrophysics of Galaxies},
  year={2015}
}
Neutral hydrogen represents the major observable baryonic constituent of galaxies that fuels the formation of stars through the transformation in molecular hydrogen. The emission of the hydrogen recombination line Halpha is the most direct tracer of the process that transforms gas (fuel) into stars. We continue to present Halpha3 (acronym for Halpha-alpha-alpha), an extensive Halpha+[NII] narrow-band imaging campaign of galaxies selected from the HI Arecibo Legacy Fast ALFA Survey (ALFALFA… 

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