Charlas
Los Seminarios y Coloquios que tendrán lugar próximamente así como las ponencias anteriores se encuentran en IAC Talks
Comisión de Seminarios: Maren Brauner, Ana Escorza Santos, Teresa Huertas Roldán, Jorge Martín Camalich, Miguel Molero González, Pablo Manuel Sánchez Alarcón
Comentarios y sugerencias: seminarios [at] iac.es (seminarios [AT] iac.es)
-
-
-
The delicate interplay between accretion, ejection and magnetism in neutron stars X-ray binariesMatter ejection, in the form of either winds or jets, is ubiquitous in accreting X-ray binaries. Although it is clear that accretion and ejection are profoundly intertwined in these types of systems, the origin and the details of such an interconnection are yet to be unraveled. This is particularly true for systems where a low-magnetized neutronDr.Alessio Marino
Aula
12 Jun 2025 - 10:30 Europe/LondonPróximas -
A chartography of spacetime around supermassive black holes with extreme-mass ratio inspiralsThe era of gravitational wave astronomy has dawned, allowing us not only to observe the universe but also to "listen" to it through gravitational waves. When a compact object ventures too close to a supermassive black hole, it becomes captured due to the emission of gravitational waves, eventually being swallowed whole as it crosses the eventDr.Pau Amaro Seoane
Aula
29 Mayo 2025 - 10:30 Europe/LondonPróximas -
IAC Breaking News
-
IAC Breaking News
-
Dust, molecules and gas in nearby AGN: JWST insights from GATOS (the Galaxy Activity, Torus, and Outflow Survey).It is widely accepted that most galaxies undergo an active phase during their evolution. The impact of the energy released by active galactic nuclei (AGN) has been proposed as a key mechanism responsible for regulating star formation (SF) by influencing the interstellar medium (ISM) of the host galaxy. Dust, gas, and molecular components are keySteph CampbellIsmael García Bernete
Aula
20 Mayo 2025 - 12:00 Europe/LondonPróximas -
Dust, molecules and gas in nearby AGN: JWST insights from GATOS (the Galaxy Activity, Torus, and Outflow Survey).It is widely accepted that most galaxies undergo an active phase during their evolution. The impact of the energy released by active galactic nuclei (AGN) has been proposed as a key mechanism responsible for regulating star formation (SF) by influencing the interstellar medium (ISM) of the host galaxy. Dust, gas, and molecular components are keySteph CampbellIsmael García Bernete
Aula
20 Mayo 2025 - 12:00 Europe/LondonPróximas