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LUNCH BREAK
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, Córdoba
EA: Chemical evolution of galaxies- Tissera
The evolution of chemical abundances in galaxies provides crucial information to study how they formed and evolved.Results in the Local Universe show that on average, star-forming gas-phase in galaxies have negative …
GA: On the Magellanic Clouds stellar clusters characterization from their integrated spectra – Simondi Romero
As part of a work carried out on Magellanic Clouds (MCs) stellar clusters (SCs), we present results in age, metallicity and reddening for Bruck 50, NGC 176, SL 164 and …
GA: Machine learning for membership determination in open clusters – Hasan
Membership of stars in clusters is very crucial in parameter determination and studies of clusters. We compare results obtained using supervised and unsupervised methods with Gaia DR2 and EDR3 data. …
GA: The dynamics of the Milky Way and the Large Magellanic Cloud – Garavito Camargo
The ongoing interaction with the Large Magellanic Cloud (LMC) is revolutionizing our view of the dynamical state of the Milky Way. The perturbations caused by the LMC open new avenues …
GA: The internal structure of clusters in the Magellanic Clouds – Rodríguez J.
The analysis of the internal structure of star clusters can provide us important information about their formation and dynamic evolution. Using data from the VISCACHA survey, we studied the spatial …
GA: Star clusters study in the inner region of the Small Magellanic Cloud – De Bortoli
We present the results of the chemical analysis of 6 star clusters in the inner region of the Small Magellanic Cloud (SMC). We used near infrared spectra obtained with GMOS …
GA: CAPOS: Distance, reddening and global metallicity determination of Bulge Globular Clusters – Villanova
Bulge Globular Cluster have always ben a challange for the determination of their distance and reddening. This is because they are affected by high differential reddening and strong field contamination. …
SH: A statistical study of the compressible energy cascade rate in the solar wind: MAVEN and PSP observations – Brodiano
Turbulence is a unique nonlinear phenomenon in fluid and plasma flows that allows the transfer of energy between different temporal and spatial scales. For instance, the solar wind is observed …
SH: Large amplitude oscillations in solar filaments – Cécere
It has been known that solar filaments show oscillations. These types of motions are normally triggered by nearby flares or jets, EIT waves and Moreton waves. In this work we …
SH: Pseudostreamer influence on flux rope evolution – Sahade
Pseudostreamers (PSs) are coronal magnetic structures formed by arcs of twin loops capped by magnetic field lines from coronal holes of the same polarity that meet at a central spine. …
IT: Virtual Workshop – Astronomy Toolkit 1.0 – Hasan
The aim of this training program is skill-building and training in Astronomy for young aspiring astronomers. The tutorial will be in two parts.Session 1: The first day will be an …
IT: Workshop – Time Domain Astronomy
Session: Friday, April 22th, 14:30-18:30 hs. Contact: Mariano Dominguez (mariano.dominguez@unc.edu.ar) Several discussion and lectures about Time Domain Astrophysics from: 14:30hs Federica Bianco (University of Delaware) TVS-ML fbianco@udel.edu15:20hs Rachel Street (Las …
IT: Virtual Workshop – Data analytics: A journey beyond the evident – Lares
Modern astronomy is a data-intensive science that requires the analysis of large volume archives. An important aspect of understanding the observations is to ask science-driven questions andto look for the …
