Abstract
The nearest, youngest groups of stars to the Sun provide important samples of age-dated stars for studying circumstellar disk evolution, imaged exoplanets, and brown dwarfs. I briefly comment on the status of the known stellar groups within 100 pc: β Pic, AB Dor, UMa, Car-Near, Tuc-Hor and β Tuc nucleus, Hyades, Col, TW Hya, Car, Coma Ber, 32 Ori, η Cha, and χ1 For. I also discuss some poorly characterized groups and non-groups. Grades for 2015 of Pass, Satisfactory, or Fail are assigned to the groups for the purposes of age-dating stars and brown dwarfs. I speculate that Tuc-Hor could have provided a supernova ∼60 pc away ∼2.2 Myr ago which showered the Earth with traces of 60Fe-bearing dust.
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Mamajek, E. E. (2015). A Pre-Gaia Census of Nearby Stellar Groups. In Proceedings of the International Astronomical Union (Vol. 10, pp. 21–26). Cambridge University Press. https://doi.org/10.1017/S1743921315006250
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