Angel R. Lopez-Sanchez

TL;DR: In this paper, the authors present new observations of IRAS 04000+5052, a Galactic HII region associated with a young stellar cluster and possibly located at the Perseus arm and find that the electron density and chemical composition of the nebula are similar to those of normal HII regions of the Galactic disk.

TL;DR: In this article, a detailed morphological, photometric and spectroscopic analysis of a sample of 20 Wolf-Rayet (WR) galaxies was performed, and the main aims were the study of the star formation and O and WR stellar populations in these galaxies and the role that interactions between low surface brightness companion objects have in the triggering of the bursts.

TL;DR: In this paper , a comparison of the merging galaxy populations detected by a sample of visual identification of tidal features around galaxies as well as spectroscopically detected close pairs of galaxies was conducted to determine whether our method of selecting merging galaxies biases our understanding of galaxy interactions.

TL;DR: In this article, the authors used the 21 cm emission line data from the DINGO-VLA project to study the atomic hydrogen gas H\,{\textsc i} of the Universe at redshifts $z < 0.1.

TL;DR: In this article, the authors performed a comprehensive analysis of a sample of 20 starburst galaxies, most of them classified as Wolf-Rayet galaxies, and analyzed the global properties of their galaxy sample using multi-wavelength data (X-ray, FUV, optical, NIR, FIR, and radio).