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20242026
most citedA new dimension in the variability of AGB stars: convection patterns size changes with pulsation

9 citations · 16 across the 8 of their papers we have counts for

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astro-ph.GA2026

Constraining young massive cluster properties with radio-continuum observations: The Arches cluster

M. Cano-González, R. Schödel, A. Alberdi +4

The Arches cluster, located in the Galactic Centre (GC) is one of the best astrophysical laboratories to study the properties of massive stars and young massive clusters (YMCs). Ho…

astro-ph.GA2026

The Nearest Galactic Nucleus: Studying the Galactic Centre with SKA-Mid

Rainer Schoedel, Antxon Alberdi, Izaskun Jiménez-Serra +24

The Galactic Centre is the nearest nucleus of a galaxy and the most extreme environment that we can observe down to physical scales of a few hundred astronomical units. There is no…

astro-ph.HE2026

Broadband multiwavelength properties of the archetypal blazar 3C 279 during the 2017 Event Horizon Telescope campaign

G. Principe, J. C. Algaba, E. Aviano +529

The archetypal blazar 3C 279 hosts a prominent relativistic jet and exhibits strong broadband variability across the electromagnetic spectrum. In April 2017, the Event Horizon Tele…

astro-ph.SR2026

Evolved massive stars and their impact on their environment

C. S. Buemi, G. Umana, C. Trigilio +15

The comprehension of the final stages of massive star evolution and their path toward the eventual supernova explosion necessarily involves the study of stellar winds and the circu…

astro-ph.GA2026

LeMMINGs VII: 5 GHz, 50 mas e-MERLIN observations of a statistically complete sample of nearby AGN

D. R. A. Williams-Baldwin, R. D. Baldi, R. J. Beswick +36

We present 5 GHz e-MERLIN radio images at 50 mas resolution of the nuclear regions of the Legacy e-MERLIN Multi-band Imaging of Nearby Galaxies survey (LeMMINGs), the deepest stati…