about
An Earth-sized planet in the habitable zone of a cool star.The three-body problem.Obliquity Variability of a Potentially Habitable Early Venus.Kepler Eclipsing Binary Stars. V. Identification of 31 Candidate Eclipsing Binaries in the K2 Engineering DatasetPlausible Compositions of the Seven TRAPPIST-1 Planets Using Long-term Dynamical SimulationsKEPLER 453 b—THE 10th KEPLER TRANSITING CIRCUMBINARY PLANETKepler-1647b: the largest and longest-period Kepler transiting circumbinary planetPlanetary candidates observed by Kepler. V. Planet sample from Q1-Q12 (36 months)Kepler eclipsing binary stars. VII. The catalog of eclipsing binaries found in the entire Kepler data setPlanetary candidates observed by Kepler. VI. Planet sample from Q1--Q16 (47 months)Instabilities in the early solar system due to a self-gravitating disk
P50
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P50
description
researcher
@en
wetenschapper
@nl
հետազոտող
@hy
name
Billy Quarles
@ast
Billy Quarles
@en
Billy Quarles
@es
Billy Quarles
@nl
type
label
Billy Quarles
@ast
Billy Quarles
@en
Billy Quarles
@es
Billy Quarles
@nl
prefLabel
Billy Quarles
@ast
Billy Quarles
@en
Billy Quarles
@es
Billy Quarles
@nl
P106
P31
P496
0000-0002-9644-8330