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Kelly Hambleton

Researcher at Villanova University

Publications -  51
Citations -  2288

Kelly Hambleton is an academic researcher from Villanova University. The author has contributed to research in topics: Binary star & Stars. The author has an hindex of 19, co-authored 46 publications receiving 1847 citations. Previous affiliations of Kelly Hambleton include University of Central Lancashire & Katholieke Universiteit Leuven.

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Kepler eclipsing binary stars. vii. the catalog of eclipsing binaries found in the entire kepler data set

Brian Kirk, +54 more
TL;DR: The final catalog of eclipsing binary systems within the 105 deg^2 Kepler field of view is presented in this paper, where the authors identify several classes of systems including those that exhibit tertiary eclipse events, systems that show clear evidence of additional bodies, heartbeat systems, and systems exhibiting only one eclipse event over the duration of the mission.
Journal ArticleDOI

Kepler Eclipsing Binary Stars. VII. The Catalog of Eclipsing Binaries Found in the Entire Kepler Data-Set

Brian Kirk, +54 more
TL;DR: The final catalog of eclipsing binary systems within the 105 square degree Kepler field of view is presented in this article, where the authors identify several classes of systems including those that exhibit tertiary eclipse events, systems that show clear evidence of additional bodies, heartbeat systems, and systems exhibiting only one eclipse event over the duration of the mission.
Journal ArticleDOI

Physics of eclipsing binaries. ii. toward the increased model fidelity

TL;DR: PHOEBE as discussed by the authors is an open source modeling code for computing theoretical light and radial velocity curves that addresses both problems by incorporating missing physics and by increasing the computational fidelity, including triangulation as a superior surface discretization algorithm, meshing of rotating single stars, light travel time effects, advanced phase computation, volume conservation in eccentric orbits, and improved computation of local intensity across the stellar surfaces.
Journal ArticleDOI

A class of eccentric binaries with dynamic tidal distortions discovered with kepler

TL;DR: In this article, a class of eccentric binary systems within the Kepler data archive that have dynamic tidal distortions and tidally induced pulsations was discovered, each having a uniquely shaped light curve that is characterized by periodic brightening or variability at timescales of 4-20 days, frequently accompanied by shorter period oscillations.
Journal ArticleDOI

Physics Of Eclipsing Binaries. II. Towards the Increased Model Fidelity

TL;DR: PHOEBE as discussed by the authors is an open source modeling code for computing theoretical light and radial velocity curves that addresses both problems by incorporating missing physics and by increasing the computational fidelity, including triangulation as a superior surface discretization algorithm, meshing of rotating single stars, advanced phase computation, volume conservation in eccentric orbits, and improved computation of local intensity across the stellar surfaces.