Congresos y charlas

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)

  • A chartography of spacetime around supermassive black holes with extreme-mass ratio inspirals
    The 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 event
    Dr.
    Pau Amaro Seoane

    Aula

    29 Mayo 2025 - 10:30 Europe/London
    Próximas
  • IAC Breaking News
    TBD
    Dr.
    José Ramón Bermejo Climent
    Dr.
    Marc Huertas Company

    Aula

    27 Mayo 2025 - 10:30 Europe/London
    Próximas
  • IAC Breaking News
    TBD
    Dr.
    José Ramón Bermejo Climent
    Dr.
    Marc Huertas Company

    Aula

    27 Mayo 2025 - 10:30 Europe/London
    Próximas
  • 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 key
    Steph Campbell
    Ismael García Bernete

    Aula

    20 Mayo 2025 - 12:00 Europe/London
    Próximas
  • 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 key
    Steph Campbell
    Ismael García Bernete

    Aula

    20 Mayo 2025 - 12:00 Europe/London
    Próximas
  • The origin of Fast X-ray Transients
    Fast X-ray Transients (FXTs) are minute-to-hours long flashes of X-rays, first discovered serendipitously in X-ray satellite data (mainly Chandra and XMM-Newton). They are proven to be caused by energetic extra-galactic phenomena. Currently, Einstein Probe is revolutionizing the field by discovering many FXTs and, crucially, by their low-latency
    Prof.
    Peter G. Jonker

    Aula

    13 Mayo 2025 - 10:30 Europe/London
    Próximas
  • TBD

    Aula

    6 Mayo 2025 - 12:30 Europe/London
    Próximas