Estudio de los campos magnéticos generados por los agujeros negros primordialesInvestigadoras desarrollaron un método con el que identificaron más de 5000 nuevas galaxiasDel polvo, venimos… Estudio de la evolución del polvo galáctico

Study of magnetic fields generated by primordial black holes

Researchers from the Institute of Theoretical and Experimental Astronomy (IATE) have participated in a theoretical study of the possibility that magnetic fields were generated from black holes that emerged in the early stages of the Universe.

Researchers developed a method with which they identified more than 5000 new galaxies

Laura Baravalle and María Victoria Alonso from the Institute of Theoretical and Experimental Astronomy (IATE) are leading an international project to search for galaxies in the direction of the disk of the Milky Way.

From dust, we come... Study of the evolution of galactic dust

A research team from the Institute for Theoretical and Experimental Astronomy (IATE), in collaboration with the Numerical Astrophysics Group in Trieste (Italy), developed computational simulations to study how dust in galaxies evolves.

Astrophysical Plasmas

figura1_1(1)The plasma is the most common state of the baryonic matter in the Universe (99%). Most of a star, the interplanetary and interstellar medium, and the ionosphere, are plasmas. The plasma can also be generated in terrestrial laboratories for industrial applications such as producing surface coatings, precision cuts in lamps, micro-motors, and plasma reactors. 

A plasma is a fluid consisting of a large number of free charged particles (globally neutral and whose kinetic energy is larger than the electrostatic potential energy between them). The charges and currents that conform a plasma are sources of the electromagnetic fields and, in turn, these fields affect the distribution of charges and currents which makes its dynamics highly nonlinear and very different from that of a neutral gas. When the magnetic fields are capable of modifying an individual particle trajectory, it is said that the plasma is magnetized. The corona is highly magnetized and therefore, several structures are observed, some of which can maintain its stability for relatively long times as dark filaments on the surface of the sun

In the group of astrophysical plasmas, our scientist perform studies about the dynamic configuration and structures of the corona through the analysis of magnetic arcs and prominences, the formation of voids that remain in the plasma due to the interaction of nonlinear waves, the formation of very energetic shock wave capable of sweeping the chromosphere along a whole quadrant, etc.

The team also analyse the interaction of stellar winds with the magnetosphere of exoplanets, and they model the morphology of supernova remnants affected by instabilities and the influence of the magnetic field. 

Galactic and Extragalactic Astronomy

The 13.8 billion years of the Universe is enough time to form giant objects, being the galaxies one of the most interesting. Galaxies are truly island universes where […]

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Stellar Astrophysics

El Universo está plagado de estrellas y la mayoría de ellas forman sistemas estelares y asociaciones. Entre los muchos sistemas estelares que pueden observarse, los cúmulos estelares (CE) se encuentran […]

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Large Scale Structure of the Universe

The large-scale structure of the Universe is the field of cosmology that studies the distribution of the matter in the Universe on the largest scales […]

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Astrophysical Plasmas

The plasma is the most common state of the baryonic matter in the Universe (99%). Most of a star, the interplanetary and interstellar medium, and the ionosphere, are plasmas […]

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Planetary Systems

Los estudios desarrollados por los integrantes del Grupo de Sistemas Planetarios buscan descifrar el origen y la evolución dinámica de planetas y cuerpos menores que orbitan el Sol u otras estrellas. […]

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