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M. Cano-Gonz'alez

3 papers hereh-index 29 citations6 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author1

Across the 3 of 3 papers where every author was matched, so the position is known.

fields
  • astro-ph.GA3

identity via Semantic Scholar / OpenAlex

works on
galactic centre 1magnetic fields 1radio survey 1square kilometre array 1star formation 1stellar remnants 1

From the 1 of 3 linked papers with an AI index.

collaborators

3 papers

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 paper proposes a large-area, multi‑wavelength continuum survey of the Galactic Centre using SKA‑Mid, covering ~2°×0.4° around Sagittarius A* and repeated deep observations of t…

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…

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