102 citations · 241 across the 5 of their papers we have counts for
7 papers
Radio observations of massive stars in the Galactic centre: The Arches Cluster
A. T. Gallego-Calvente, R. Schoedel, A. Alberdi +8
We present high-angular-resolution radio observations of the Arches cluster in the Galactic centre, one of the most massive young clusters in the Milky Way. The data were acquired…
The Milky Way's nuclear star cluster: Old, metal-rich, and cuspy
R. Schödel, F. Nogueras-Lara, E. Gallego-Cano +3
(abridged) We provide Ks photometry for roughly 39,000 stars and H-band photometry for about 11,000 stars within a field of about 40"x40", centred on Sgr A*. In addition, we provid…
GALACTICNUCLEUS: A high-angular-resolution JHKs imaging survey of the Galactic centre III. Evidence for wavelength dependence of the extinction curve in the near-infrared
Francisco Nogueras-Lara, Rainer Schödel, Nadine Neumayer +4
The characterisation of the extinction curve in the near infrared (NIR) is fundamental to analyse the structure and stellar population of the Galactic centre (GC), whose analysis i…
New constraints on the structure of the nuclear stellar cluster of the Milky Way from star counts and MIR imaging
E. Gallego-Cano, R. Schödel, F. Nogueras-Lara +5
The Milky Way nuclear star cluster (MWNSC) is a crucial laboratory for studying the galactic nuclei of other galaxies, but its properties have not been determined unambiguously unt…
First results from a large-scale proper motion study of the Galactic Centre
B. Shahzamanian, R. Schödel, F. Nogueras-Lara +4
Proper motion studies of stars in the centre of the Milky Way have been typically limited to the Arches and Quintuplet clusters and to the central parsec. Here, we present the firs…
Variability of the near-infrared extinction curve towards the Galactic centre
Francisco Nogueras-Lara, Rainer Schödel, Francisco Najarro +4
Due to the extreme extinction towards the Galactic centre ( mag), its stellar population is mainly studied in the near-infrared (NIR) regime. Therefore, a proper ana…