Loading view.
Ongoing
LUNCH BREAK
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, Córdoba
EA: On the influence of halo mass accretion history on galaxy properties and assembly bias – Montero Dorta
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, CórdobaHalo 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 …
EA: EMPIRE: A new semi-empirical model for the Galaxy-Halo connection – Rodriguez Puebla
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 …
EA: Dark-matter-deficient galaxies in the Illustris-TNG simulations – Tau
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 …
EA: Spiral galaxies with ring structures – Alonso S.
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 …
EA: Bar properties in dwarf barred galaxies from Virgo – Cuomo
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 …
EA: MaNGA/SDSS-IV: Archaeological reconstruction of the radial and global growth of galaxies – Ávila-Reese
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, CórdobaThe 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, …
EA: Gas shocks around galaxy clusters – Rost
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, CórdobaGas 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 …
EA: A deep near-infrared view of the Ophiuchus galaxy cluster – Coldwell
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, CórdobaThe 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 …
EA: Kinematics of the Local Group gas and galaxies in the Hestia simulations – Biaus
We investigate the kinematic properties of gas and galaxies in the Local Group (LG) using a suite of high-resolution simulations performed by the Hestia (High-resolution Environmental Simulations of The Immediate …
EA: The physical origin and impact of stellar-gas misalignments in galaxies from the CIELO simulation – Casanueva
We use zoom-in galaxies from the Chemo-dynamIcal propertiEs of gaLaxies and the cOsmic web (CIELO) cosmological hydrodynamical simulation to study the physical origin and structural impact of the kinematic misalignment …
EA: Nearby galaxies — insights into galaxy evolution – Menendez Delmestre
Galaxies in the local universe are a fossil record of events in the distant universe and present critical constraints on the physical processes underlying the formation and evolution of galaxies. …
IT: New and upcoming astronomical instrumentation: opportunities for collaboration between Latin American astronomers – Signorini Goncalves
The next decade will see a true revolution in astronomical instrumentation, starting with the launch and first light of the James Webb Space Telescope and extending to the new thirty-meter-class …
CG: Virtual Workshop – Gravitational Waves – Vieira Gomes
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 …
