19 citations · 25 across the 5 of their papers we have counts for
6 papers
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…
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…
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…
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…
The formation history of our Galaxy's nuclear stellar disc constrained from HST observations of the Quintuplet field
R. Schoedel, F. Nogueras-Lara, M. Hosek +9
Until recently it was thought that the nuclear stellar disc at the centre of our Galaxy was formed via quasi-continuous star formation over billions of years. However, an analysis…
Detecting hot stars in the Galactic centre with combined near- and mid-infrared photometry
M. Cano-González, R. Schödel, F. Nogueras-Lara
{The Galactic centre (GC) is a unique astrophysical laboratory to study the stellar population of galactic nuclei because it is the only galactic nucleus whose stars can be resolve…