722 citations · 3.3k across the 43 of their papers we have counts for
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Discovery of the pre-main-sequence eclipsing binary MML 48
Y. Gómez Maqueo Chew, L. Hebb, H. C. Stempels +12
We present the discovery of the eclipsing binary MML 48, which is a member of Upper Centaurus Lupus, has an associated age of 16 Myr, and is composed of two young, low-mass stars.…
Absolute dimensions of solar-type eclipsing binaries. NY Hya: A test for magnetic stellar evolution models
T. C. Hinse, O. Baştürk, J. Southworth +29
The binary star NY Hya is a bright, detached, double-lined eclipsing system with an orbital period of just under five days with two components each nearly identical to the Sun and…
Revisiting the Membership, Multiplicity, and Age of the Beta Pictoris Moving Group in the Gaia Era
Rena A. Lee, Eric Gaidos, Jennifer van Saders +2
Determining the precise ages of young (tens to a few hundred Myr) kinematic (``moving") groups is important for placing star, protoplanetary disk, and planet observations on an evo…
TESS Hunt for Young and Maturing Exoplanets (THYME) IX: a 27 Myr extended population of Lower-Centaurus Crux with a transiting two-planet system
Mackenna L. Wood, Andrew W. Mann, Madyson G. Barber +35
We report the discovery and characterization of a nearby (~ 85 pc), older (27 +/- 3 Myr), distributed stellar population near Lower-Centaurus-Crux (LCC), initially identified by se…
A Stringent Test of Magnetic Models of Stellar Evolution
Guillermo Torres, Gregory A. Feiden, Andrew Vanderburg +1
Main-sequence stars with convective envelopes often appear larger and cooler than predicted by standard models of stellar evolution for their measured masses. This is believed to b…
Gaia Gaps and the Physics of Low-Mass Stars. I. The Fully Convective Boundary
Gregory A. Feiden, Khian Skidmore, Wei-Chun Jao
The Gaia M-dwarf gap is a significant under-density of stars observed near in a color-magnitude diagram for stars within 200 pc of the Sun. It has been proposed that t…