Giant planets around two intermediate-mass evolved stars and confirmation of the planetary nature of HIP 67851c

@article{Jones2015GiantPA,
  title={Giant planets around two intermediate-mass evolved stars and confirmation of the planetary nature of HIP 67851c},
  author={M. I. Jones and James S. Jenkins and Patricio Rojo and Claudio H. F. Melo},
  journal={Astronomy and Astrophysics},
  year={2015},
  volume={580}
}
Context. Precision radial velocities are required to discover and ch aracterize planets orbiting nearby stars. Optical and near infrared spectra that exhibit many hundreds of absorption lines can allow the m s −1 precision levels required for such work. However, this means that studies have generally focused on solar-type dwarf stars. After the main-sequence, intermediate-mass star s (former AF stars) expand and rotate slower than their progenitors, th us thousands of narrow absorption lines… 
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