Chemical complexity in the interstellar medium and star formation group

My research focuses on the processes that determine the evolution of circumstellar disks around low- and high-mass protostars, and their potential impact on the ability of the disk to form planets.

I am currently doing my PhD at the Center for Astrobiology under the direction of Izaskun Jiménez-Serra and Nuria Huélamo, where we explore the effect of photoionization, protostellar winds and jets, and binary companions on the evolution of disks. 

Prior to this, I graduated in Physics from Universidad de Valencia in 2018 and got a Master's Degree in Astrophysics from Universidad Autónoma de Madrid in 2019.

For my investigation, I analyze observations from radio to optical wavelengths, from single dish and interferometric facilities, namely ALMA, VLTI, VLA, SMA, GTC and IRAM 30m. I am also an experienced user of MORELI, a 3D non-LTE radiative transfer code that predicts the radio continuum and hydrogen radio recombination line emission from star forming regions, for current and future telescopes such as the SKA. 

I am first author of three peer-reviewed articles, and have presented my work in four conferences and three seminars.