output
19952026
most citedDigital Twin: Enabling Technologies, Challenges and Open Research

2.9k citations

Showing 2025 · astro-ph.SRShow all

20 papers · 2 filters

astro-ph.SR2025★ 5 cited

The stellar activity-rotation-age relationship under the lens of asteroseismology

C. Pezzotti, J. Bétrisey, G. Buldgen +6

In low-mass stars, the connection between magnetic activity, rotation period, and age provides key insights into the functioning of dynamos. Fully understanding the activity-rotati…

astro-ph.SR2025

Newborn jet in the symbiotic system R Aquarii

T. Liimets, D. P. K. Banerjee, M. Santander-García +12

R Aquarii (R Aqr) is a well-known symbiotic binary that has attracted renewed interest during its recent periastron passage, an event that occurs only once every about 40 years. Th…

astro-ph.SR2025

The EBLM Project XVIII. 3D Obliquities of Five Low-Mass Eclipsing Binaries

Becca Spejcher, David V. Martin, Jake Pandina +17

The formation of tight stellar binaries remains an unsolved problem. There is too much angular momentum in a collapsing and fragmenting protostellar cloud to form a stellar binary…

astro-ph.SR2025★ 1 cited

3D Synthetic Convective Velocity Fields to Initialise Core-Collapse Supernova Simulations from 1D Progenitors

Vishnu Varma, Bernhard Mueller, Raphael Hirschi

Core-collapse supernovae (CCSNe) are among the most energetic and complex astrophysical phenomena, requiring threedimensional (3D) simulations to capture their intricate explosion…

astro-ph.SR2025★ 22 cited

A high fraction of close massive binary stars at low metallicity

H. Sana, T. Shenar, J. Bodensteiner +74

At high metallicity, a majority of massive stars have at least one close stellar companion. The evolution of such binaries is subject to strong interaction processes, heavily impac…

astro-ph.SR2025

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.…