The HR 1614 moving group is not a dissolving cluster

@article{Kushniruk2020TheH1,
  title={The HR 1614 moving group is not a dissolving cluster},
  author={I. Kushniruk and Thomas Bensby and Sofia Feltzing and Christian L Sahlholdt and Diane K. Feuillet and Luca Casagrande},
  journal={Astronomy \& Astrophysics},
  year={2020}
}
Context. The HR 1614 is an overdensity in velocity space and has for a long time been known as an old (∼2 Gyr) and metal-rich ([Fe/H] ≈ +0.2) nearby moving group that has a dissolving open cluster origin. The existence of such old and metal-rich groups in the solar vicinity is quite unexpected since the vast majority of nearby moving groups are known to be young. Aims. In the light of new and significantly larger data sets than ever before (astrometric, photometric, and spectroscopic), we aim… 
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