activity
20112022
most citedA comprehensive approach to analyzing the XMM-Newton data of Seyfert 1 galaxies

12 citations · 12 across the 4 of their papers we have counts for

collaborators

7 papers

astro-ph.GA2025

Deriving the abundance distribution of HII galaxies using sulphur as tracer: Exploring the high-metallicity end

Marta Gavilán, Ángeles I. Díaz, Sandra Zamora

The main objective of this work is to derive the distribution of the the metal content of HII galaxies using sulphur as an abundance tracer. This increases the metallicity range th…

astro-ph.GA2022

Physical properties of circumnuclear ionizing clusters: NGC 7742

S. Zamora, Ángeles I. Díaz

We have analyzed the circumnuclear ring of the spiral galaxy NGC7742 in order to understand its formation and evolution. We have obtained gaseous abundances, characterized the inte…

astro-ph.GA2022

Using Sulfur as metallicity tracer in galaxies

Ángeles I. Díaz

We review the present methodology for the use of Sulfur as global metallicity tracer in galaxies, which allows performing a complete abundance analysis using mainly the red to near…

astro-ph.GA2022

Interstellar reddening correction using He I lines

S. Zamora, Ángeles I. Díaz, Elena Terlevich +1

We present a method to derive the logarithmic extinction coefficient in optical wavelengths using the emission lines of HeI. Using this procedure we can avoid selection biases when…

astro-ph.GA2019

2D-Galactic chemical evolution: the role of the spiral density wave

Mercedes Mollá, Sheillah Wekesa, Oscar Cavichia +6

We present a 2-dimensional chemical evolution code applied to a Milky Way type galaxy, incorporating the role of spiral arms in shaping azimuthal abundance variations, and confront…

astro-ph.GA2018

The time evolution of the Milky Way's oxygen abundance gradient

M. Mollá, Á. I. Díaz, O. Cavichia +5

We study the evolution of oxygen abundance radial gradients as a function of time for the Milky Way Galaxy obtained with our {\sc Mulchem} chemical evolution model. We review the r…