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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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Journal Article

Circumnuclear structure and kinematics in the active galaxy NGC 6951

TL;DR: In this paper, a study of the central structure and kinematics of the galaxy NGC 6951 is presented by means of broad band B 0 IJK images and high resolution high dispersion longslit spec- troscopy, together with archival HST WFPC2 V and NICMOS2 J and H images.
Posted Content

The massive Stellar Content in Starburst Galaxies and its Impact on Galaxy Evolution

TL;DR: In this paper, the massive stellar content in starburst galaxies and their evolutionary state is derived based on the analysis of their integrated light with evolutionary synthesis models, in a selfconsistent way using the continuum and stellar wind resonance lines in the ultraviolet, the photospheric H Balmer and HeI lines and the nebular emission lines at optical wavelengths.
Journal ArticleDOI

The Mice at play in the CALIFA survey: A case study of a gas-rich major merger between first passage and coalescence

Vivienne Wild, +56 more
TL;DR: In this paper, optical integral field spectroscopy (IFS) observations of the Mice, a major merger between two massive (>10^11Msol) gas-rich spirals NGC4676A and B, observed between first passage and final coalescence.
Journal ArticleDOI

The stellar population and the evolutionary state of HII regions and starburst galaxies

TL;DR: In this article, the stellar content and evolutionary state of RHII s and starbursts from their ultraviolet and optical integrated light were derived from a prototypical RHII (NGC 604) and nuclear starburst (NIC 7714).
Journal ArticleDOI

Detection of a Super Star Cluster as the Ionizing Source in the Low Luminosity AGN NGC 4303

TL;DR: In this article, the authors proposed that at least some LLAGNs in spirals could be understood as the result of the combined ionizing radiation emitted by an evolving SSC and a black hole (BH) accreting with low radiative efficiency, coexisting in the inner few parsecs region.