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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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Showing astro-ph.GAShow all

5 papers · 1 filter

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.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…

astro-ph.GA2025

A multi-frequency, multi-epoch radio continuum study of the Quintuplet cluster with the Very Large Array

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

The Quintuplet cluster, located in the Galactic centre, is one of the few young massive clusters in the Milky Way. It allows us to study dozens of massive, post main sequence stars…

astro-ph.GA2024★ 2 cited

A multi-frequency, multi-epoch radio continuum study of the Arches cluster with the VLA

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

The Arches cluster, one of the most massive clusters in the Milky Way, is located about 30 pc in projection from the central massive black hole. With its high mass, young age, and…