Extragalactic archaeology provides new clues about the formation of the galaxies

An artistic illustration that combines a real image of a galaxy with a representation of the stellar orbits within it, to show how the study of the movements of stars allows us to reconstruct the history of galaxies.
Advertised on

An international review article in which IAC researcher Jesús Falcón Barroso is a contributor, explains how the study of stellar populations in galaxies outside the Milky Way and the Local Group, using techniques which are called “extragalactic archaeology”, permits the reconstruction of the processes of formation and evolution of those galaxies. This article has been published in the Annual Review of Astronomy & Astrophysics, one of the most prestigious journals in this field, to which only five researchers of the IAC have contributed during the lifetime of the Institute.

How did the galaxies we see in the Universe today form and evolve? The article "Extragalactic Archaeology: The Assembly History of Galaxies from Dynamical and Stellar Population Models" answers this question by reviewing the latest advances in extragalactic archaeology: a discipline that seeks to reconstruct the history of galaxies from the detailed study of their stars and internal motions. This work is co-authored by IAC astrophysicist Jesús Falcón-Barroso,along with Glenn van de Ven (University of Vienna) and Mariya Lyubenova (European Southern Observatory, ESO). The article has been published by invitation in the Annual Review of Astronomy & Astrophysics, a publication reserved for internationally renowned researchers.

“Nearby galaxies act as true cosmic laboratories,” explains Falcón-Barroso. “By combining dynamical models with stellar population models and data provided by integral field spectroscopy instruments, we can uncover the ‘fossil records’ of their assembly history and better understand how they form and evolve in a cosmological context,” he adds.

The paper reviews advances in the use of dynamical models to measure mass distributions of galaxies—including their central black holes and dark matter halos—and stellar population models to decipher the ages and chemical compositions of stars. It also highlights the potential of their combined application to unravel the imprint of past processes, such as galaxy mergers or the formation of inner disks.

The research also stresses the role of nearby galaxies as bridges to knowledge: their proximity allows us to obtain detailed maps of their stellar properties and dynamics, with a resolution impossible to achieve in more distant galaxies. These results constitute a fundamental reference for calibrating cosmological simulations and relating detailed studies of the Local Group—which includes the Milky Way—with observations of galaxies in the early Universe.

"This type of reviews not only synthesizes current knowledge but also outlines future directions for work in a rapidly expanding field. This publication reinforces the IAC’s international reach and its leadership in the study of galaxy evolution," Falcón-Barroso emphasizes.

A publication of reference in Astrophysics

Founded in 1963, Annual Review of Astronomy & Astrophysics publishes exclusively invited review articles, in which international experts summarize the current state of a research area and highlight its challenges and prospects. It is the highest-impact journal in the field of astrophysics for this type of work, with an exceptionally high citation rate.

In its more than six decades of history, only five IAC researchers have had their work published there: Carme Gallart and Antonio Aparicio (2005), Javier Trujillo and Tanausú del Pino (2022) and now, Jesús Falcón-Barroso (2025).

 

Article: Glenn van de Ven, Jesús Falcón-Barroso and Mariya Lyubenova: “Extragalactic Archaeology: The Assembly History of Galaxies from Dynamical and Stellar Population Models”, Annual Review of Astronomy & Astrophysics, Vol. 63:259-297, 2025. DOI: https://doi.org/10.1146/annurev-astro-052622-025659

Related projects
Group members
Traces of Galaxy Formation: Stellar populations, Dynamics and Morphology
We are a large, diverse, and very active research group aiming to provide a comprehensive picture for the formation of galaxies in the Universe. Rooted in detailed stellar population analysis, we are constantly exploring and developing new tools and ideas to understand how galaxies came to be what we now observe.
Anna
Ferré Mateu
ExGal-Twin logo
ExGal-Twin: Excellence in Galaxies - Twinning the IAC
This Twinning action aims to strengthen the research and networking capacity, profile and impact of the Instituto de Astrofísica de Canarias (IAC) in the area of galaxies through the development of strategic alliances of this regionally leading institute in an Outermost Region of the EU (OR), with three excellent European partners. An initial SWOT
Johan Hendrik
Knapen Koelstra
Related news
The colour-magnitude diagram of 151 galaxies observed by CALIFA. For each galaxy it is shown a true-color image created using the B (blue), V (green) and R (red) band reconstructed images extracted from the CALIFA datacubes. In this diagram, the galaxies
The Calar Alto Legacy Integral Field Area survey (CALIFA survey),  that counts with the participation of the Instituto de Astrofísica de Canarias (IAC), announces today its first public release of data, offering an unprecedentedly detailed view of one hundred galaxies in the local universe with ample opportunities for scientific study. Together with the data release, two technical publications authored by members of the CALIFA collaboration have been made publicly available, describing the data and showing some of their scientific applications. The Calar Alto Legacy Integral Field Area
Advertised on
First results of Herschel and the HerMES extragalactic survey.
ESA's Herschel Space Observatory was launched on 14 May 2009. After a short commissioning and performance verification period, the science demonstration observations started in September 2009. Herschel is now carrying out routine science observations. The three instruments (SPIRE, PACS and HIFI) are working extremely well. The IAC is part of the SPIRE and PACS instrument consortia and has contributed flying hardware and software. The first results of the many Herschel Key Projects were presented at the ESLAB 2010 symposium in ESTEC (May 2010) and have been published in July 2010 in a special
Advertised on
Imagen artística de las primeras supernovas de la Vía Láctea. La estrella Pristine 221.8781+9.7844 se formó a partir del material eyectado por estas primeras supernovas. Crédito: Gabriel Pérez, SMM (IAC).
An international team of researchers, including David S. Aguado, Jonay González and Carlos Allende Prieto of the Instituto de Astrofísica de Canarias (IAC), has found a star with extremely low metallicyt, one of the oldest in the Milky Way, and for that reason an excellent messenger from the early universe.
Advertised on