Add to ORKGWe present our ongoing work on integral field spectroscopy of three prototypical HII galaxies: IIZw70, IIZw71 and IZw18. The data are mainly used to study the ionized gas and stellar clusters. Our main goal is to investigate the presence of spatial variations in ionization structure indicators, physical conditions and gaseous metal abundances, in these galaxies. Maps of the relevant emission lines and a preliminary analysis of the ionization structure are presented for IIZw70
Artículo de publicación ISIContext. Hii regions in galaxies are the sites of star formation, so they...
We propose a methodology to perform a self-consistent analysis of the physical properties of the emi...
Integral field spectroscopy is presented for star-forming regions in M33. A central area of 300 × 50...
International audienceAims.We performed an integral field spectroscopic study for the HII galaxy IIZ...
Aims.We performed an integral field spectroscopic study for the HII galaxy IIZw70 to investigate th...
International audienceWe present a detailed 2D study of the ionized ionized interstellar medium (ISM...
A detailed spectroscopic study, from lambda 3700 A to 1 um, has been performed for a sample of 34 HI...
We analyse the spectroscopic properties of thousands of H _Π regions identified in 38 face-on spiral...
Here we review some of our more recent results on the observed properties of HII regions using Integ...
Premio a la mejor tesis doctoral en Astronomía y Astrofísica del año 2017 (Sociedad Española de Astr...
In this thesis, wide-field 2D spectroscopy is employed in order to characterise the nebular properti...
We analyse the spectroscopic properties of thousands of H ii regions identified in 38 face-on spiral...
Symposium A30 (Astronomy in Focus XXX) August 2018 , p. 258 presented at IAU XXX General Assembly, V...
We present a detailed study of the physical properties of the nebular material in four starforming k...
Long-slit spectroscopy has been obtained for a sample of 22 blue dwarf galaxies selected in the dire...
Artículo de publicación ISIContext. Hii regions in galaxies are the sites of star formation, so they...
We propose a methodology to perform a self-consistent analysis of the physical properties of the emi...
Integral field spectroscopy is presented for star-forming regions in M33. A central area of 300 × 50...
International audienceAims.We performed an integral field spectroscopic study for the HII galaxy IIZ...
Aims.We performed an integral field spectroscopic study for the HII galaxy IIZw70 to investigate th...
International audienceWe present a detailed 2D study of the ionized ionized interstellar medium (ISM...
A detailed spectroscopic study, from lambda 3700 A to 1 um, has been performed for a sample of 34 HI...
We analyse the spectroscopic properties of thousands of H _Π regions identified in 38 face-on spiral...
Here we review some of our more recent results on the observed properties of HII regions using Integ...
Premio a la mejor tesis doctoral en Astronomía y Astrofísica del año 2017 (Sociedad Española de Astr...
In this thesis, wide-field 2D spectroscopy is employed in order to characterise the nebular properti...
We analyse the spectroscopic properties of thousands of H ii regions identified in 38 face-on spiral...
Symposium A30 (Astronomy in Focus XXX) August 2018 , p. 258 presented at IAU XXX General Assembly, V...
We present a detailed study of the physical properties of the nebular material in four starforming k...
Long-slit spectroscopy has been obtained for a sample of 22 blue dwarf galaxies selected in the dire...
Artículo de publicación ISIContext. Hii regions in galaxies are the sites of star formation, so they...
We propose a methodology to perform a self-consistent analysis of the physical properties of the emi...
Integral field spectroscopy is presented for star-forming regions in M33. A central area of 300 × 50...