R
Rosa M. González Delgado
Researcher at Spanish National Research Council
Publications - 69
Citations - 6534
Rosa M. González Delgado is an academic researcher from Spanish National Research Council. The author has contributed to research in topics: Galaxy & Stellar population. The author has an hindex of 25, co-authored 58 publications receiving 6012 citations. Previous affiliations of Rosa M. González Delgado include Space Telescope Science Institute.
Papers
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Nuclear activity and massive star formation in the low luminosity AGN NGC4303: Chandra X-ray observations
E. Jimenez-Bailon,Maria Santos-Lleo,Jose Miguel Mas-Hesse,Matteo Guainazzi,Luis Colina,Miguel Cerviño,Rosa M. González Delgado +6 more
TL;DR: In this paper, the authors present evidence of the coexistence of either an AGN or an ultraluminous X-ray source (ULX), together with a young super stellar cluster in the 3 central parsecs of NGC4303.
Journal ArticleDOI
On the Origin of the Ultraviolet Continuum in Seyfert 2 Galaxies
Luis Colina,Luis Colina,María Luisa García Vargas,Rosa M. González Delgado,J. Miguel Mas-Hesse,Enrique Pérez,Enrique Pérez,Antxon Alberdi,Antxon Alberdi,Alfred Krabbe +9 more
TL;DR: In this paper, the authors presented the first direct empirical evidence that the UV flux emitted by galaxies having a Seyfert 2-type nucleus surrounded by a circumnuclear star-forming ring is dominated by radiation coming from clusters of young hot stars distributed along the star forming ring.
Journal ArticleDOI
On the importance of the few most massive stars: the ionizing cluster of NGC 588
L. Jamet,Enrique Pérez,Miguel Cerviño,Grazyna Stasinska,Rosa M. González Delgado,José M. Vílchez +5 more
TL;DR: In this article, a double analysis of the ionizing cluster in NGC 588, a giant HII region (GHR) in the outskirts of the nearby galaxy M33, is presented.
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O VI + Lyβ + C II from Starburst and Poststarburst Galaxies. I. Stellar Library and Evolutionary Synthesis Profiles
TL;DR: In this article, an evolutionary synthesis model of a stellar population in the far-ultraviolet spectra is presented, based on observations of O and B stars collected with Copernicus and the Hopkins Ultraviolet Telescope (HUT).