Opening and Registration
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, Córdoba, ArgentinaRegistration for in-person attendees and welcoming speach
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SA: Chemical Abundances in Planetary Nebulae: Collisionally Excited Lines vs. Recombination Lines – Peña
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 …
SA: Automated classification of eclipsing binary systems in the VVV Survey – Daza Perilla
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 …
SA: Strong non-dipolar magnetic fields in millisecond pulsars? – Pelle
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 …
COFFEE BREAK (mornings)
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, Córdoba, Argentina
SA: Formation and Evolution of central stars of Planetary Nebulae – Miller Bertolami
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 …
SA: Plasma Correction in the “Cosine Relation” for Pulsar Pulse Profile – Briozzo
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 …
SA: Exploration of magnetic activity indices in M dwarfs – Oviedo
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 …
PS: Regolith ejection on the asteroid Didymos due to its fast rotation – Trógolo
(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 …
PS: Orbital evolution of circumbinary planets due to creep tides – Zoppetti
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 …
LUNCH BREAK
Auditorio Mirta Mosconi Francisco N de Laprida 854, X5000BGR Córdoba, Córdoba, Argentina
SA: The physical and chemical signatures of young protostars and planet-forming disks. – Artur V
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 …
CG: Virtual Workshop – Extended Mass Distributions of Primordial Black Holes and Primordial Magnetogenesis
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 …
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 …
