papers

Publications (13)

astro-ph2004

The tidally disturbed luminous compact blue galaxy Mkn 1087 and its surroundings

Angel R. Lopez-Sanchez, Cesar Esteban, Monica Rodriguez

We present new broad-band optical and near-infrared CCD imaging together with deep optical intermediate-resolution spectroscopy of Mkn 1087 and its surrounding objects. We analyze…

astro-ph.CO2011

The intriguing HI gas in NGC 5253: an infall of a diffuse, low-metallicity HI cloud?

Angel R. Lopez-Sanchez, Baerbel Koribalski, Janine van Eymeren +4

(Abridged) We present new, deep HI line and 20-cm radio continuum data of the very puzzling blue compact dwarf galaxy NGC 5253, obtained with the ATCA as part of the `Local Volume…

astro-ph.CO2009

The environment of nearby Blue Compact Dwarf Galaxies

Angel R. Lopez-Sanchez, Barbel Koribalski, Janine van Eymeren +3

We are obtaining deep multiwavelength data of a sample of nearby blue compact dwarf galaxies (BCDGs) combining broad-band optical/NIR and H photometry, optical spectroscopy and…

astro-ph.CO2010

The ionized gas at the center of IC 10: A possible localized chemical pollution by Wolf-Rayet stars

Angel R. Lopez-Sanchez, Adal Mesa-Delgado, Luis Lopez-Martin +1

We present results from integral field spectroscopy with the Potsdam Multi-Aperture Spectrograph at the 3.5m telescope at Calar Alto Observatory of the intense star-forming region…

astro-ph2008

Massive star formation in Wolf-Rayet galaxies: I. Optical and NIR photometric results

Angel R. Lopez-Sanchez, Cesar Esteban

(Abridged) We have performed a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show the presence of a substantial population of massive stars. The…

astro-ph.IM2020

White Paper on MAAT@GTC

Francisco Prada, Robert Content, Ariel Goobar +41

MAAT is proposed as a visitor mirror-slicer optical system that will allow the OSIRIS spectrograph on the 10.4-m Gran telescopio CANARIAS (GTC) the capability to perform Integral F…

astro-ph.CO2009

Massive star formation in Wolf-Rayet galaxies: II. Optical spectroscopy results

Angel R. Lopez-Sanchez, Cesar Esteban

(Abridged) We have performed a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show the presence of a substantial population of very young massive…

astro-ph.CO2010

Massive star formation in Wolf-Rayet galaxies. IV: Colours, chemical composition analysis and metallicity-luminosity relations

Angel R. Lopez-Sanchez, Cesar Esteban

(Abridged) We performed a multiwavelength analysis of a sample of starburst galaxies that show the presence of a substantial population of very young massive (WR) stars. Here we pr…

astro-ph.GA2021

Electron temperature fluctuations in Seyfert galaxies

Rogemar A. Riffel, Oli L. Dors, Angela Krabbe +1

We use Gemini GMOS-IFU observations of three luminous nearby Seyfert galaxies (Mrk79, Mrk348 and Mrk607) to estimate the electron temperature () fluctuations in the inne…

astro-ph2007

On the abundance discrepancy problem in HII regions

Jorge Garcia-Rojas, Cesar Esteban

The origin of the abundance discrepancy is one of the key problems in the physics of photoionized nebula. In this work, we analize and discuss data for a sample of Galactic and ext…

astro-ph2004

IRAS 04000+5052: A not so compact, not so metal-poor HII region

Cesar Esteban, Luis Lopez-Martin, Angel R. Lopez-Sanchez +2

We present new observations of IRAS 04000+5052, a Galactic HII region associated with a young stellar cluster and possibly located at the Perseus arm. Contrary to previous claims,…

astro-ph.CO2010

Massive star formation in Wolf-Rayet galaxies. III: Analysis of the O and WR populations

Angel R. Lopez-Sanchez, Cesar Esteban

(Abridged) We perform a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show the presence of a substantial population of Wolf-Rayet (WR) stars. In…

astro-ph.CO2010

Massive star formation in Wolf-Rayet galaxies: IV b. Using empirical calibrations to compute the oxygen abundance

Angel R. Lopez-Sanchez, Cesar Esteban

We have performed a comprehensive multiwavelength analysis of a sample of 20 starburst galaxies that show a substantial population of very young massive stars, most of them classif…