This work is the first study on the 3D shape of starbursting extremely metal-poor galaxies (XMPs; a galaxy is said to be an XMP if its ionized gas-phase...
The Shape of III Zw2 Hα Line: Evidence of Keplerian Relativistic Disk
We have analyzed the shape of III Zw2 Hα emission line observed at Isaac Newton telescope. A model with a Keplerian relativistic disk plus one emission region...
The shape of the Galactic abundance gradient of oxygen from deep spectra of H II regions
We present results of an ongoing project dedicated to reassess the shape of the radial abundance gradient of O in the Milky Way based on deep spectroscopy of H...
The shape of the ionised gas abundance distribution in spiral galaxies
In this contribution we review some of the most relevant results of the PhD thesis awarded with the XIV SEA PhD prize in 2018. The thesis is aimed at...
Swift, a dedicated gamma-ray burst (GRB) satellite with ultrarapid slewing capability, and a suite of ground-based (ESO) telescopes have recently achieved a...
We propose a wide-area, high latitude, imaging survey to trace the evolution of dusty, star-forming galaxies, evolved stellar populations, and AGN, as a...