collaborators

10 papers

astro-ph.IM2026

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

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

The paper summarizes 70 science cases for the proposed NASA Habitable Worlds Observatory, outlining the observational needs across four scientific pillars and detailing required ca…

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…

astro-ph.SR2026

Magnetic fields in Massive Star-Forming Regions (MagMaR). VIII. Magnetic field overrun by gravity in GGD 27's accretion streamers

M. Fernández-López, J. A. López-Vázquez, J. M. Girart +20

Context. Accretion streamers connected to protostellar disks and/or envelopes are thought to transport material across several thousand of au. Whether the motions of the gas compri…

physics.flu-dyn2026

Submesoscale and boundary layer turbulence under mesoscale forcing in the upper ocean

S. Peng, S. Silvestri, A. Bodner

The interaction among quasi-geostrophic mesoscale eddies, submesoscale fronts, and boundary layer turbulence (BLT) is a central problem in upper ocean dynamics. We investigate thes…

astro-ph.HE2026

X-ray stellar feedback in low-metallicity starbursts: Insights from the template starburst galaxy ESO 338-IG04 and its halo

M. Chatzis, L. M. Oskinova, S. Reyero Serantes +7

The X-ray output of low-metallicity starburst galaxies is a key component of stellar feedback, tracing the processes responsible for gas ionization and chemical enrichment. The int…

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…