Zobrazeno 1 - 10
of 37
pro vyhledávání: '"Roberto B. Menezes"'
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 496:943-958
In this work, we continue the study of the central region of NGC 613 by da Silva et al. (2020), by analysing the stellar and gas kinematics and the stellar archaeology in optical and near-infrared data cubes. The high spatial resolution of the Gemini
Publikováno v:
Monthly Notices of the Royal Astronomical Society. 492:5121-5140
In this paper, we report a detailed study with a variety of data from optical, near-infrared, X-ray, and radio telescopes of the nuclear region of the galaxy NGC 613 with the aim of understanding its complexity. We detected an extended stellar emissi
The detailed study of nuclear regions of galaxies is important because it can help understanding the active galactic nucleus (AGN) feedback mechanisms, the connections between the nuclei and their host galaxies, and ultimately the galaxy formation pr
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::88b3c68b993e2a165521f306d88c5264
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
We present a study of the central 200 pc of the galaxy NGC 6951, SAB(rs)bc, an active twin of the Milky Way, at a distance of 24 Mpc. Its nucleus has been observed in the optical with the GMOS-IFU, showing an outflow, and with the HST/ACS, revealing
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::dbbbd81ed0aab0a44f0c2cef9b5d05cd
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
We analysed the centre of NGC 1566, which hosts a well-studied active galactic nucleus (AGN), known for its variability. With the aid of techniques such as Principal Component Analysis Tomography, analysis of the emission-line spectra, channel maps,
Publikováno v:
Proceedings of the International Astronomical Union. 15:364-365
Active Galactic Nuclei (AGN) are objects in which a supermassive black hole is fed by gas and, as this generates energy, can ionise the environment and interact with it by jets and winds. This work is focused on the processes of feeding and feedback
Publikováno v:
Proceedings of the International Astronomical Union. 15:450-451
We present the first results of the Deep Integral Field Spectroscopy View of Nuclei of Galaxies (DIVING3D) survey, obtained from the analysis of the nuclear emission-line spectra of a sub-sample we call mini-DIVING3D, including all southern galaxies
Autor:
Roberto B. Menezes, Rogério Riffel, D. Ruschel-Dutra, Juliana C. Motter, Marlon R. Diniz, J. E. Steiner, Tiago V. Ricci, Rogemar A. Riffel, Natacha Z. Dametto, L. G. Dahmer-Hahn, Thaisa Storchi-Bergmann
Publikováno v:
Proceedings of the International Astronomical Union. 15:427-428
We analyzed the inner 320 × 535 pc2 of the elliptical galaxy NGC 1052 with integral field spectroscopy, both in the optical and in the near-infrared (NIR). The stellar population analysis revealed a dominance of old stellar populations from the opti
Autor:
J. E. Steiner, Roberto B. Menezes
We analyze optical data cubes of the nuclear regions of two late-type galaxies, NGC 908 and NGC 1187, obtained with the Integral Field Unit of the Gemini Multi-Object Spectrograph. Both data cubes show stellar structures consistent with double nuclei
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::704fca763f65313f8b7d468a2f0abe6c
http://arxiv.org/abs/1901.06703
http://arxiv.org/abs/1901.06703
Autor:
Rogemar A. Riffel, L. G. Dahmer-Hahn, Thaisa Storchi-Bergmann, N. Z. Dametto, D. Ruschel-Dutra, J. E. Steiner, Marlon R. Diniz, Tiago V. Ricci, Juliana C. Motter, R. A. Riffel, Roberto B. Menezes
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
We map the optical and near-infrared (NIR) emission-line flux distributions and kinematics of the inner 320$\times$535pc$^2$ of the elliptical galaxy NGC1052. The integral field spectra were obtained with the Gemini Telescope using the GMOS-IFU and N
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4860e895d5a5360ef34022d95886e61c