Análisis exhaustivo de eyecciones de plasma solarMigraciones galácticas: ¿cómo se pueblan los cúmulos?Esperando el primer contacto

Comprehensive analysis of solar plasma ejections

Researchers from the Institute of Theoretical and Experimental Astronomy (IATE), together with an international team, published an article in which, based on observations, the deviations of solar material ejections are studied.

Galactic migrations: How are clusters populated?

José Benavides, a doctoral fellow at the Institute for Theoretical and Experimental Astronomy (IATE), Mario Abadi, a researcher at the same institute, and Laura Sales, from the University of California, published an article in which they analyze, based on computer simulations, how the galaxies arrive to clusters and what their interactions are like once they are inside.

Waiting for the first contact

Marcelo Lares, researcher at IATE (CONICET - UNC), in collaboration with José Funes (CONICET - Universidad Católica de Córdoba) and Luciana Gramajo (CONICET - Observatorio Astronómico de Córdoba), developed and simulated a model that allows analyzing the probability of contacts between civilizations that are in different points of our galaxy.

Corresponding Researchers

IATE also has Corresponding Researchers (Resolution 1351, 2015, CONICET). They are active Argentine and foreign scientific and technological researchers from institutions outside Argentina that have strong links with IATE. With recognized prestige and with important contributions to science and technology, they are involved with our institution as PHD advisors, participating in research projects, teaching courses, and any other activity that contributes to the development of scientific and technological research in Argentina.

Mario C. Díaz : Profesor Titular de Física y Astronomía, Universidad Texas Valle del Rio Grande y Director del Centro de Astronomía de Ondas Gravitacionales

Mario C. Díaz

Profesor Titular de Física y Astronomía, Universidad Texas Valle del Rio Grande y Director del Centro de Astronomía de Ondas Gravitacionales

mario.diaz@utrgv.edu
Nelson Padilla : Profesor Asistente, Pontificia Universidad Católica de Chile.

Nelson Padilla

Assistant Professor, Pontificia Universidad Católica de Chile.

npadilla@astro.puc.cl
Patricia Tissera : Profesora Titular, Universidad Andrés Bello, Chile

Patricia Tissera

Professor, Universidad Andrés Bello, Chile

patricia.tissera@unab.cl

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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