Estudio de oscilaciones en filamentos solares

Explican el origen de un tipo de galaxias

PISCIS: una herramienta de ciencia ciudadana para analizar imágenes astronómicas

Study of oscillations in solar filaments

An international team of researchers from the Astrophysical Plasmas area of the Institute of Theoretical and Experimental Astronomy (IATE), based on computational simulations, analyzed and modelled how large solar prominences are affected by waves from the solar corona.

Explaining the origin of a type of galaxy

The breakthrough published in the prestigious journal Nature Astronomy was achieved by an international team of scientists led by José Benavides and Mario Abadi, from the National University of Córdoba (UNC) and CONICET, and Laura Sales, from the University of California, Riverside.

PISCIS: a citizen science tool for analysing astronomical images

A team from Instituto de Astronomía Teórica y Experimental (IATE), led by Vanessa Daza, Germán Alfaro and José Benavides, developed an interactive platform in which experts and non-experts can collaborate in the processing of astronomical data.

Authorities

Director: Dr. Diego Garcia Lambas

Vicedirector: Dr. Hernán Muriel

Directive Consil:

Titular Researchers	Cic Suplentes
Dra. Cinthia Ragone Figueroa	Dr. Dante paz
Dr. Carlos Valotto	Dr. Federico Stasyzsin
Dr. Julián Martínez	Dra. Ana Laura O’Mill
Dra. María Laura Ceccarelli
Dra. Valeria Coenda
Dr. Carlos Donzelli
CPA Titular	Alternate CPA
Ing. Horacio Rodríguez	Dario Graña
Titular Fellow	Alternate Fellow
Lic. Germán Alfaro	Lic. Abril Sahade

Comunicación Institucional: Facundo Rodríguez

Instituto de Astronomía Teórica y Experimental

Study of oscillations in solar filaments

Explaining the origin of a type of galaxy

PISCIS: a citizen science tool for analysing astronomical images

Authorities

Galactic and Extragalactic Astronomy

Stellar Astrophysics

Large Scale Structure of the Universe

Astrophysical Plasmas

Planetary Systems