activity
20032026
most citedAn Extended Grid of Nova Models: II. The Parameter Space of Nova Outbursts

530 citations · 1.5k across the 32 of their papers we have counts for

collaborators

32 papers

astro-ph.SR2026

Orbital and stellar parameter determination of eclipsing Cep pulsators

C. I. Eze, G. Handler, F. Kahraman Aliçavuş +2

Eclipsing binaries provide precise constraints on stellar properties and evolution, making those hosting Cep pulsators particularly valuable for characterising massive pulsatin…

astro-ph.GA2026

Magnetic Fields in Massive Star-forming Regions (MagMaR). IX. Radiative Torque Alignment and Disruption in NGC6334I

Vineet Rawat, Thiem Hoang, Patricio Sanhueza +18

Intense radiation from high-mass stars is expected to significantly affect dust grain alignment and evolution through RAdiative Torques (RATs). We investigate this effect in a mass…

astro-ph.EP2026

A Cross-Laboratory Comparison Study of Titan Haze Analogs: Surface Energy II

Eric C. Austin, Xinting Yu, Chao He +10

The organic haze particles on Titan play important roles in atmospheric cloud formation and aerosol-lake interactions. These processes are strongly influenced by the surface energy…

astro-ph.IM2026

Early Exploration of the Scientific Discovery Space for the Habitable Worlds Observatory

Courtney D. Dressing, Danica Adams, Evelyne Alecian +324

The Habitable Worlds Observatory (HWO) is a future NASA flagship mission concept identified by the Astro2020 Decadal Survey as the highest priority for large space missions. HWO sh…

cond-mat.str-el2026

Single crystal growth, structural and magnetic properties of CeZnGa

Danila Sokratov, H. Cein Mandujano, Ram Kumar +9

The tetragonal BaAl () parent structure underpins a diverse family of materials exhibiting novel phenomena, including nematic superconductivity, topological semimetalli…

physics.flu-dyn2026

A theoretical model for oceanic submesoscales under next-order effects of strain and turbulence

Shirui Peng, Abigail Bodner

Submesoscale currents in the oceanic mixed layer, comprising fronts, eddies, and filaments, are characterized by Rossby numbers (Ro). These features, which constant…