activity
20162022
most citedCarbon and oxygen in HII regions of the Magellanic Clouds: abundance discrepancy and chemical evolution

96 citations · 129 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2022★ 28 cited

The homogeneity of chemical abundances in H II regions of the Magellanic Clouds

G. Domínguez-Guzmán, M. Rodríguez, J. García-Rojas +3

We use very deep spectra obtained with the Ultraviolet-Visual Echelle Spectrograph at the Very Large Telescope to derive physical conditions and chemical abundances of four H II re…

astro-ph.GA2019★ 4 cited

Chemical abundances and temperature structure of H II regions

G. Domínguez-Guzmán, M. Rodríguez, C. Esteban +1

We use a sample of 37 H II regions with high quality spectra to study the behavior of the relative abundances of several elements as a function of metallicity. The sample includes…

astro-ph.GA2017

Spatial distribution of carbon and oxygen abundances in the Magellanic Clouds

L. Toribio San Cipriano, C. Esteban, G. Domínguez-Guzmán +1

We present chemical abundances of carbon and oxygen in the Large and Small Magellanic Clouds from optical spectra of H II regions. We analyse the behaviour of the O/H, C/H and C/O…

astro-ph.GA2017★ 96 cited

Carbon and oxygen in HII regions of the Magellanic Clouds: abundance discrepancy and chemical evolution

L. Toribio San Cipriano, G. Domínguez-Guzmán, C. Esteban +5

We present C and O abundances in the Magellanic Clouds derived from deep spectra of HII regions. The data have been taken with the Ultraviolet-Visual Echelle Spectrograph at the 8.…

astro-ph.GA2017★ 1 cited

The abundances of O, N, S, Cl, Ne, Ar, and Fe in H II regions of the Magellanic Clouds

G. Domínguez-Guzmán, M. Rodríguez, C. Esteban +1

We use very deep spectra obtained with the Ultraviolet-Visual Echelle Spectrograph in the Very Large Telescope in order to determine the physical conditions, the chemical abundance…

astro-ph.GA2016

Study on the Abundance Discrepancy Problem in the Magellanic Clouds

L. Toribio San Cipriano, C. Esteban, G. Domínguez-Guzmán +1

We present chemical abundances of carbon (C) and oxygen (O) in the Large and Small Magellanic Clouds from deep and high-quality optical spectra of HII regions. The data have been t…