Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Suzi Diniz"'
Autor:
Suzi Diniz, J. E. Steiner, Rogemar A. Riffel, Rogério Riffel, Miriani Griselda Pastoriza, J. A. Hernandez-Jimenez, Tiago V. Ricci
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 used Gemini Multi-Object Spectrograph (GMOS) in the Integral Field Unit mode to map the stellar population, emission line flux distributions and gas kinematics in the inner kpc of NGC 5044. From the stellar populations synthesis we found that the
Autor:
Ruth Gruenwald, Alberto Rodríguez-Ardila, Suzi Diniz, Lucimara P. Martins, Ronaldo Eustáquio de Souza
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
Recent models show that TP-AGB stars should dominate the NIR spectra of populations 0.3 to 2 Gyr old, leaving unique signatures that can be used to detect young/intermediate stellar population in galaxies. However, no homogeneous database of star-for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6be389ec25b650bd20abd4aa1ed749c3
http://arxiv.org/abs/1302.3853
http://arxiv.org/abs/1302.3853
Autor:
Alberto Rodríguez-Ardila, Lucimara P. Martins, Ronaldo Tavares de Souza Souza, Suzi Diniz, Rogério Riffel
Publikováno v:
Scopus-Elsevier
The near-infrared spectral region is becoming a very useful wavelength range to detect and quantify the stellar population of galaxies. Models are developing to predict the contribution of TP-AGB stars, that should dominate the NIR spectra of populat
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::6f0d3846f4eaa151b272ac3229aa484e