File:UscotCTIO 55 mapgraph.jpg
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Summary
[edit]Vector-point diagrams comparing the proper motions of our discoveries in Upper Scorpius (USco, filled red stars) and Upper Centaurus–Lupus (UCL, open red stars) to those of Sco–Cen objects from the literature. Left: we show our proper motions for objects in the Upper Sco lists of LM12, Dawson et al. (2014), and Rizzuto et al. (2015; black circles, labeled "L+D+R" in the legend) that are not saturated in PS1 and have reliable proper motion fits, and the proper motions of known and candidate Upper Sco members from UKIDSS GCS (Lodieu 2013, blue diamonds). Right: proper motions of F-type stars in Upper Sco (black filled circles) and UCL (black open circles) from Pecaut et al. (2012). All six of our Sco–Cen discoveries have proper motions consistent with all literature sources. From: https://iopscience.iop.org/article/10.3847/1538-4357/aa5df0
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current | 14:57, 18 October 2024 | 2,052 × 1,046 (520 KB) | Foxy Husky (talk | contribs) | Vector-point diagrams comparing the proper motions of our discoveries in Upper Scorpius (USco, filled red stars) and Upper Centaurus–Lupus (UCL, open red stars) to those of Sco–Cen objects from the literature. Left: we show our proper motions for objects in the Upper Sco lists of LM12, Dawson et al. (2014), and Rizzuto et al. (2015; black circles, labeled "L+D+R" in the legend) that are not saturated in PS1 and have reliable proper motion fits, and the proper motions of known and candidate Up... |
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