Zobrazeno 1 - 5
of 5
pro vyhledávání: '"Juliana C. Motter"'
Autor:
Juliana C. Motter, Marlon R. Diniz, Rogemar A. Riffel, D. Ruschel-Dutra, L. G. Dahmer-Hahn, R. A. Riffel, Tiago V. Ricci, Miriani Griselda Pastoriza, N. Z. Dametto, Thaisa Storchi-Bergmann, Alberto Rodríguez-Ardila
The merger remnant NGC 34 is a local luminous infrared galaxy (LIRG) hosting a nuclear starburst and a hard X-ray source associated with a putative, obscured Seyfert~2 nucleus. In this work, we use adaptive optics assisted near infrared (NIR) integra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3f28eadc3731476b123f977210d03da6
http://arxiv.org/abs/2107.09731
http://arxiv.org/abs/2107.09731
Autor:
J. E. Steiner, Tiago V. Ricci, João P. V. Benedetti, D. Ruschel-Dutra, Miriani Griselda Pastoriza, Rogemar A. Riffel, Juliana C. Motter, Rogério Riffel
Publikováno v:
Proceedings of the International Astronomical Union. 15:418-420
We mapped the stellar population and emission gas properties in the nuclear region of NGC 6868 using datacubes extracted with Gemini Multi-Object Spectrograph (GMOS) in the Integral Field Unit (IFU) mode. To obtain the star-formation history of this
Autor:
Rogério Riffel, Miriani Griselda Pastoriza, Juliana C. Motter, Rogemar A. Riffel, Tiago V. Ricci, Alberto Rodríguez-Ardila, D. Ruschel-Dutra, L. G. Dahmer-Hahn, N. Z. Dametto, Thaisa Storchi-Bergmann, Marlon R. Diniz
Publikováno v:
Proceedings of the International Astronomical Union. 15:355-356
Understanding the interplay between the phenomena of active galactic nuclei (AGN) and starbursts remains an open issue in studies of galaxy evolution. The galaxy NGC 34 is the remnant of the merger of two former gas-rich disc galaxies and it also hos
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:
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