The 3D structure of the Virgo cluster from H-band Fundamental Plane and Tully—Fisher distance determinations

@article{Gavazzi1999The3S,
  title={The 3D structure of the Virgo cluster from H-band Fundamental Plane and Tully—Fisher distance determinations},
  author={G. Gavazzi and A. Boselli and M. Scodeggio and D. Pierini and E. Milano and Italy. and Laboratoire d' Astronomie Spatiale and Marseille and France. and Eső and G. B. Munchen and H Germany and M. F. Kernphysik and Heidelberg},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={1999},
  volume={304},
  pages={595-610}
}
We undertook a surface photometry survey of 200 galaxies in the Virgo cluster (complete to B<14.0 mag) carried out in the near-infrared (NIR) H band. Combining velocity dispersion measurements from the literature with new spectroscopic data for 11 galaxies, we derive distances of 59 early-type galaxies using the Fundamental Plane (FP) method. The distances of another 75 late-type galaxies are determined using the Tully--Fisher (TF) method. For this purpose we use the maximum rotational velocity… Expand
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