activity
20052023
most citedKepler Eclipsing Binary Stars. I. Catalog and Principal Characterization of 1879 Eclipsing Binaries in the First Data Release

529 citations · 1.7k across the 35 of their papers we have counts for

collaborators

36 papers

astro-ph.SR2023

Living with a Red Dwarf: X-ray, UV, and Ca II Activity-Age Relationships of M Dwarfs

Scott G. Engle

The vast majority of stars in the nearby stellar neighborhood are M dwarfs. Their low masses and luminosities result in slow rates of nuclear evolution and minimal changes to the s…

astro-ph.SR2023

Living With a Red Dwarf: The Rotation-Age Relationship of M Dwarfs

Scott G. Engle, Edward F. Guinan

Age is a fundamental stellar property, yet for many stars it is difficult to reliably determine. For M dwarfs it has been notoriously so. Due to their lower masses, core hydrogen f…

astro-ph.SR2022

X-rays in Cepheids: Identifying Low-Mass Companions of Intermediate-Mass Stars

Nancy Remage Evans, Scott Engle, Ignazio Pillitteri +12

X-ray observations have been made of a sample of 20 classical Cepheids, including two new observations (Polaris and {\it l} Car) reported here. The occurrence of X-ray flux around…

astro-ph.SR2021★ 5 cited

X-rays in Cepheids: XMM-Newton Observations of Aql

Nancy Remage Evans, Ignazio Pillitteri, Pierre Kervella +13

X-ray bursts have recently been discovered in the Cepheids Cep and Dor modulated by the pulsation cycle. We have obtained an observation of the Cepheid Aql with the XMM…

astro-ph.SR2020

Hubble Space Telescope Snapshot Survey for Resolved Companions of Galactic Cepheids: Final Results

Nancy Remage Evans, H. Moritz Guenther, Howard E. Bond +13

Cepheids in multiple systems provide information on the outcome of the formation of massive stars. They can also lead to exotic end-stage objects. This study concludes our survey o…

astro-ph.SR2020★ 5 cited

X-ray Observations of the Peculiar Cepheid V473 Lyr Identify A Low-Mass Companion

Nancy Remage Evans, Ignazio Pillitteri, Laszlo Molnar +17

V473 Lyr is a classical Cepheid which is unique in having substantial amplitude variations with a period of approximately 3.3 years, thought to be similar to the Blazhko variations…