Opening and Registration
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, Córdoba, ArgentinaRegistration for in-person attendees and welcoming speach
Friends of Friends Hybrid Meeting 2022
XI Friends of Friends Meeting – Linking astronomy and friends in Córdoba
Registration for in-person attendees and welcoming speach
Chemical abundances of planetary nebulae (PNe) help us to understand several processes of the nucleosynthesis of the progenitor star. Elements such as He, C, and N can be processed in …
In this study, we use a recently published catalogue of one hundred EBSs, classified by fine-tuning theoretical models according to contact, detached or semi-detached classes. We describe the method implemented …
It has been recently suggested that the millisecond pulsar PSR J0030+0451 has a significant off-centered non-dipolar magnetic field component. This has been deduced via statistical inference methods on the shape …
Since their discovery in 1764 our ideas for the formation of Planetary Nebulae (PNe) have improved continuously. The basic picture traced in the mid-twentieth century of PNe being transition objects …
We will study the trajectories of photons emitted by a pulsar with emphasis on the chromatic effects derived from the presence of a plasmatic environment. We will show how to …
During the last decades, M stars have gained substantial interest in the search for exoplanets due not only to the high occurrence of terrestrial-type planets but also to the greater …
(65803) Didymos is the binary Near Earth Asteroid target of the DART (NASA)/LICIA (ASI) andHera (ESA) missions. It orbits the Sun with a semi-major axis of 1.64 AU, and it …
In this work, we present the results of applying the creep tide model (Ferraz Mello 2013) to the orbital evolution of circumbinary planets. This model allow us to consider stiff …
In the process of low-mass star formation, a protoplanetary disk is assembled around the young star and planets will form within this disk. Therefore, the chemical composition of the early …
This workshop consists of a series of short lectures and hands-on activities on the topic of Primordial Black Holes (PBHs). In particular, on understanding and computing extended mass functions of …
Gravitational waves are solutions of General Relativity (GR) both at linear and fully nonlinear levels, and have been directly found recently. These can be addressed from different approaches: linearisation for …
In 2015, the first direct detection of a gravitational wave (GW) by the two ground-based LIGO interferometers opened a new era for gravitational-wave astrophysics. Since then, more than 90 events …
Gravastars are exotic compact objects alternative to black holes. In the context of alternative theories of gravity, they present relevant signatures. Thus, we shall present the gravastar solutions of a …
A novel 4-dimensional Einstein-Gauss-Bonnet (4D EGB) gravity has been proposed that asserts to bypass Lovelock’s theorem and to result in a non-trivial contribution to the gravitational dynamics in four-dimensional spacetime. …
In this work, we have studied a Convolutional Neural Network (CNN) called WienerNet to apply the Wiener Filter to noisy CMB (Cosmic Microwave Background) maps. We present how these neural …
Galaxy clusters are important cosmological probes since their abundance and spatial distribution are directly linked to structure formation on large scales. The principal uncertainty source on the cosmological parameter constraints …
The relationship between the integrated Hβ line luminosity and the velocity dispersion of the ionized gas of HII galaxies (HIIGs) and giant HII regions (GHIIRs) has been known for a …
In this talk, we show a framework to consistently model the spatial distribution and time evolution of dark matter, gas, and galaxies, in the Large Scale Structure of the universe. …
We present well-posedness results for two particular theories aiming to model large-scale magnetic field amplification. We report on the existence of spurious modes when the electromotive force is linear in …
We implement a universal method for renormalizing AdS gravity actions applicable to arbitrary higher curvature theories in up to five dimensions. The renormalization procedure considers the extrinsic counterterm for Einstein-AdS …
During the 21st century, gravitational lensing turned from a curious relativistic effect used by some cosmologists into a mainstream astrophysical tool. Each year we witness new discoveries exploring the different …
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 …
This workshop consists of a series of short lectures and hands-on activities on the topic of Primordial Black Holes (PBHs). In particular, on understanding and computing extended mass functions of …
Using the EAGLE hydrodynamical simulation, we explore what drives the formation of giant (and massive), low surface brightness galaxies of the Kind of Malin 1. We investigate on the role …
We explored the nature of Low Surface Brightness galaxies (LSBGs) in the local universe, by using a set of simulated galaxies from TNG100. We compared galaxy properties at z=0 such …
In this work is performed a photometric analysis for a sample of 101 galaxies in the near infrared (NIR) bands of 2MASS (J, H, Ks) with the goal of estimating …
Properties of galaxies and their evolution are strongly affected by their local environment. It has also been explored how the local environment affects the active galactic nuclei (AGN) phenomena. These …
Using a set of well--behaved novel statistical parameters we study the alignment signal of galactic spins with respect to the centre of voids identified in the TNG-300 simulation. We explore …
Being the lowest-surface-brightness galaxies known, Ultra-diffuse galaxies (UDGs) are among the most intriguing objects in the Universe. Since their rediscovery a few years ago, different mechanisms have been proposed to …
In this work, we study the relationship between star formation activity and the active galactic nucleus phenomenon, known as AGN-starburst connection. For this purpose, we use a catalogue of galaxy …
We perform a systematic validation of the models of the pairwise velocities of galaxies based on the pair conservation of cosmic tracers. The equation that governs the dynamics of pairwise …
The formation and stability of collisionless self-gravitating systems are long-standing problems, which date back to the work of D. Lynden-Bell on violent relaxation and extend to the issue of virialization …
Stellar streams are a consequence of the tidal forces produced by a host galaxy on its satellites (i.e. globular clusters and dwarf spheroidals). As the self-gravity of stellar streams is …
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 …
During the 21st century, gravitational lensing turned from a curious relativistic effect used by some cosmologists into a mainstream astrophysical tool. Each year we witness new discoveries exploring the different …
Fundamentos básicos de Linux, Iniciación en el uso de la consola, conexión a un sistema remoto y uso del sistema de colas.Shell, comandos, filesystem, procesos, conexión SSH, sistema de colas …
This workshop consists of a series of short lectures and hands-on activities on the topic of Primordial Black Holes (PBHs). In particular, on understanding and computing extended mass functions of …
Halo assembly bias is the secondary dependence of the clustering of dark matter haloes on their assembly histories at fixed halo mass. This established dependence is expected to manifest itself …
In this talk, I will introduce EMPIRE, a new consistent semi-empirical model for the Galaxy-Halo connection. EMPIRE uses the mass assembly of dark matter halos and a battery of observations …
In the standard model of galaxy formation, galaxies form within a halo of dark matter, which is the component that dominates the matter budget of the Universe. Surprisingly, some recent …
In this talk we will present a statistical analysis of different characteristics of ringed spiral galaxies with the aim of assessing the effects of rings on disk galaxy properties. We …
We study 5 barred dwarf galaxies located in the Virgo cluster to understand the effect of the environment on the formation and evolution of their bars. We measure the properties …
The MaNGA survey has observed >10,000 local galaxies from SDSS using the integral field spectroscopy technique. By applying inverse stellar population synthesis (fossil record method) to their spatially resolved spectra, …
Gas shocks occur naturally around galaxy clusters, among several processes, the high-speed infalling gas deaccelerates and heats up near the centre of the cluster. The material infalling towards these objects …
The Ophiuchus cluster of galaxies, the 2nd brightest X-ray cluster in the sky, has been relatively poorly studied. It is located at low latitudes in the direction of the Galactic …