The Herschel Virgo Cluster Survey - XX. Dust and gas in the foreground Galactic cirrus

@article{Bianchi2016TheHV,
  title={The Herschel Virgo Cluster Survey - XX. Dust and gas in the foreground Galactic cirrus},
  author={Stefano Bianchi and Carlo Giovanardi and M. W. L. Smith and Jacopo Fritz and Jonathan Ivor Davies and Martha P. Haynes and Riccardo Giovanelli and Maarten Baes and Marco Bocchio and Samuel Boissier and M{\'e}d{\'e}ric Boquien and Alessandro Boselli and Viviana Casasola and Christopher J. R. Clark and I. De Looze and S. di Serego Alighieri and Marco Grossi and A. P. Jones and Thomas M. Hughes and Leslie K. Hunt and S. Madden and Laura Magrini and Ciro Pappalardo and Nathalie Ysard and Stefano Zibetti},
  journal={Astronomy and Astrophysics},
  year={2016},
  volume={597}
}
We study the correlation between far-infared/submm dust emission and atomic gas column density in order to derive the properties of the high Galactic latitude, low density, Milky Way cirrus in the foreground of the Virgo cluster of galaxies. Dust emission maps from 60 to 850 um are obtained from SPIRE observations carried out within the Herschel Virgo Cluster Survey, complemented by IRAS-IRIS and Planck-HFI maps. Data from the Arecibo legacy Fast ALFA Survey is used to derive atomic gas column… 

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