activity
20042026
most cited(Sub)stellar companions shape the winds of evolved stars

132 citations · 1.1k across the 50 of their papers we have counts for

collaborators

53 papers

astro-ph.GA2026

Advancing extragalactic spectral line studies with the Square Kilometre Array Observatory

Jacco Th. van Loon, Viviana Casasola, Manuela Bischetti +6

We present an overview of the Square Kilometre Array Observatory (SKAO) science potential in the area of extragalactic spectral lines besides 21-cm neutral hydrogen. It highlights…

astro-ph.GA2026

Cosmic Rulers: Masers as Tools for Probing Structure in the Galaxy and Beyond, from AU to kpc

Kazi L. J. Rygl, Anna Bartkiewicz, Olga Bayandina +9

Maser emission provides an unique window into astronomical sources across vast spatial scales - from tens to hundreds of astronomical units around protostars and evolved stars up t…

astro-ph.GA2026

Measuring Magnetic Fields Near and Far with the SKA via the Zeeman Effect

Timothy Robishaw, Marta Nowotka, Tao-Chung Ching +7

Zeeman splitting in spectral lines -- both in emission and absorption -- provides direct estimates of magnetic field strength and direction in magnetized gas in our own Milky Way a…

astro-ph.SR2026

ATOMIUM: Inner circumstellar envelopes of oxygen-rich AGB stars as revealed by highly excited SiO lines

B. Pimpanuwat, S. Etoka, M. D. Gray +14

Silicon monoxide (SiO) traces the physical conditions and dynamics in the circumstellar envelopes (CSEs) of AGB stars. We present high-resolution ALMA Band 6 observations of highly…

astro-ph.SR2025★ 5 cited

Evidence for the Keplerian orbit of a close companion around a giant star

Mats Esseldeurs, Leen Decin, Joris De Ridder +31

Close companions influence stellar evolution through tidal interactions, mass transfer, and mass loss effects. While such companions are detected around young stellar objects, main…

astro-ph.SR2025

3D Maser polarization simulation for J=1-0 SiO masers in the circumstellar envelope of an AGB star

M. Phetra, M. D. Gray, K. Asanok +4

SiO masers from AGB stars exhibit variability in intensity and polarization during a pulsation period. This variability is explained by radiative transfer and magnetic properties o…