Timothy D. Brandt's scientific contributions
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Citations
... In the HGCA (Brandt 2018(Brandt , 2019, HD 92987 can be easily identified as a star with significant proper-motion variability, as previously found by Frankowski et al. (2007) and discussed in Section 2.1. The measured difference between the Gaia and Hip-Gaia proper motions is ∼14.4 mas yr −1 , equivalent to a tangential velocity difference of ∼3000 m s −1 for the star's parallax. ...