Organizational unit: RESEARCH DIVISION

Email
coordinacion.investigacion [at] iac.es
Headquarter
Headquarters
Description
The Research Division engages in the elaboration and development of research projects in astrophysics and its related fields. To meet its objectives, the Division is organized with a managerial structure and services dedicated to facilitating and channeling the development of its research activities.
  • Job
    IAC POSTDOCTORAL FELLOWSHIP Stellar Populations 2026
    The IAC (Tenerife) invites applications for ONE postdoctoral contract to work on the project linked to the line of research “Traces of galaxy formation: stellar...
  • Project
    Kinematic, Structural and Composition Studies of the Interstellar and Intergalactic Media
    The basic objective of the broject is to investigate the evolution of galaxies by deepening our understanding of the interaction between the insterstellar...
  • Project
    Magnetism, Polarization and Radiative Transfer in Astrophysics
    Magnetic fields pervade all astrophysical plasmas and govern most of the variability in the Universe at intermediate time scales. They are present in stars...
  • Project
    Milky Way and Nearby Galaxies
    The general aim of the project is to research the structure, evolutionary history and formation of galaxies through the study of their resolved stellar...
  • Project
    Molecular Gas and Dust in Galaxies Across Cosmic Time
    Two of the most fundamental questions in astrophysics are the conversion of molecular gas into stars and how this physical process is a function of environments...
  • Project
    Morphology and dynamics of the Milky Way
    This project consists of two parts, each differentiated but both complementary: morphology and dynamics. Detailed study of the morphology of the Milky Way...
  • Project
    Nuclear Activity in Galaxies: a 3D Perspective from the Nucleus to the Outskirts
    The group has two main research lines. First, the study of quasar-driven outflows in luminous and nearby obscured active galactic nuclei (AGN) and the impact...
  • Project
    Nucleosynthesis and molecular processes in the late stages of Stellar Evolution
    Low- to intermediate-mass (M < 8 solar masses, Ms) stars represent the majority of stars in the Cosmos. They finish their lives on the Asymptotic Giant Branch...
  • Project
    Numerical Astrophysics: Galaxy Formation and Evolution
    How galaxies formed and evolved through cosmic time is one of the key questions of modern astronomy and astrophysics. Cosmological time- and length-scales are...