Context. Although there have been numerous studies of chemical abundances in the Galactic bulge, the central two degrees have been relatively unexplored due to the heavy and variable interstellar extinction, extreme stellar crowding, and the presence of complex foreground disk stellar populations.Aims. In this paper we discuss the metallicity...
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July 2019 (v1)Journal articleUploaded on: December 4, 2022
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January 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
October 2021 (v1)Journal article
It has long been suspected that powerful radio sources may lower the efficiency with which stars form from the molecular gas in their host galaxy, however so far, alternative mechanisms, in particular related to the stellar mass distribution in the massive bulges of their host galaxies, have not been ruled out. We present new,...
Uploaded on: December 4, 2022 -
August 2023 (v1)Journal article
We present an analysis of new VLT/MUSE optical imaging spectroscopic data of 2MASX J23453268–0449256 (J2345–0449), a nearby ( z = 0.0755) massive ( M stellar = 4 × 10 11 M ⊙ ) spiral galaxy. This is a particularly interesting source for a study of active galactic nucleus (AGN) feedback since it hosts two pairs of bright, giant radio jets and a...
Uploaded on: November 25, 2023 -
June 2021 (v1)Journal article
Context. The nuclear stellar disc (NSD) is, together with the nuclear star cluster (NSC) and the central massive black hole, one of the main components in the central parts of our Milky Way. However, until recently, only a few studies of the stellar content of the NSD have been obtained owing to extreme extinction and stellar crowding.Aims. We...
Uploaded on: December 4, 2022 -
2007 (v1)Journal article
Context: To reveal the origin of mid-infrared radiation from the core of Centaurus A, we carried out interferometric observations with the MID-infrared Interferometer (MIDI) at ESO's VLTI telescope array. Aims: Observations were obtained with four baselines between unit telescopes of the VLTI, two of them roughly along the radio axis and two...
Uploaded on: December 4, 2022