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20012026
most citedPatterns of photometric and chromospheric variation among Sun-like stars: A 20-year perspective

229 citations · 1.7k across the 45 of their papers we have counts for

collaborators

46 papers

astro-ph.SR2026

A Pre-Main Sequence Binary Viewed Through its Circumbinary Disk: A New Phase for KH 15D

Catrina M. Hamilton, Adi B. Chacko, George A. Carson +16

The binary T Tauri system, KH 15D, is poised to provide unprecedented detail of gas and ices located between 3-5 AU of its circumbinary disk over the next few years. We analy…

astro-ph.EP2026

NEO Colors from The Mission Accessible Near-Earth Object Survey (MANOS)

Nicholas Moskovitz, Theodore Kareta, Samantha Hemmelgarn +13

We present spectro-photometric griz colors for 189 near-Earth objects (NEOs) collected by the Mission Accessible Near-Earth Object Survey (MANOS). Data acquisition involved non-sim…

astro-ph.SR2024

The Discovery of Three Galactic Wolf-Rayet Stars

Laurella C. Marin, Philip Massey, Brian A. Skiff +1

Wolf-Rayet stars (WRs) are evolved massive stars in the brief stage before they undergo core collapse. Not only are they rare, but they also can be particularly difficult to find d…

astro-ph.SR2024

Haro 5-2: A New Pre-Main Sequence Quadruple Stellar System

Bo Reipurth, C. Briceno, T. R. Geballe +9

We have discovered that the Halpha emission line star Haro 5-2, located in the 3-6 Myr old Ori OB1b association, is a young quadruple system. The system has a 2+2 configuration wit…

astro-ph.SR2024

The Stellar Content of the Young Open Cluster Berkeley 50 (IC 1310)

Meghan Speckert, Philip Massey, Brian A. Skiff

We observed the Galactic open cluster Berkeley 50 in order to determine its stellar content, distance, and age. We obtained UBV photometry of 1145 stars in a 12.3' 12.3' f…

astro-ph.SR2024

The POKEMON Speckle Survey of Nearby M Dwarfs. III. The Stellar Multiplicity Rate of M Dwarfs within 15 pc

Catherine A. Clark, Gerard T. van Belle, Elliott P. Horch +8

M dwarfs are ubiquitous in our galaxy, and the rate at which they host stellar companions, and the properties of these companions, provides a window into the formation and evolutio…