At the Institute of Nuclear Science (ICN-UNAM), we conduct a wide range of research in astrophysics. Our work explores topics like star formation, high-energy astrophysics, computational astrophysics and data science, and astrobiology. We aim to better understand the universe, from the birth of stars to the conditions that could support life on other planets. The ICN team consists of passionate researchers, students, and postdocs working together to answer some of the biggest questions in science.
Astrophysical research is conducted by people from different departments at the ICN, engaging in transdisciplinary research across various fields of physics and chemistry. The departments involved are High Energy Physics, Plasma Physics and Interaction of Radiation with Matter, and Gravitation and Field Theory. We are:
Miguel Alcubierre | Black holes, gravitational waves, dark matter, numerical relativity |
Fabio De Colle | Gamma-ray bursts, supernovae, TDEs, high-energy transients, computational astrophysics and data science |
Alejandro Esquivel | Star formation, computational astrophysics, interstellar medium |
Diego López Cámara | Gamma-ray bursts, computational astrophysics, high-energy transients |
Verónica Lora | Star formation |
Néstor Ortiz | Neutron stars, black holes, gravitational waves, general relativity |
Hernando Quevedo | General relativity, quantum gravity |
Ary Rodríguez | Massive star clusters, Atomic and molecular flows, photoionization models, Hydrodynamics, Interstellar Medium |
Sarira Sahu | Neutrino Astrophysics, Cosmic Rays, Gamma-ray Bursts, Ultra-high Energy Cosmic Rays |
Marcelo Salgado | Black Holes, Cosmology, General and Numerical Relativity, Alternative Theories of Gravitation |
Antígona Segura | Astrobiology, Exoplanet Atmospheres, Biosignatures, Planetary Habitability |
Juan Claudio Toledo Roy | Biosignals, Scientific Computing, Hydrodynamics, Astrophysical Plasmas |
Pablo Velázquez | Astrophysical Flows, Supernova Remnants, thermal and non-thermal emission, MHD |
Diana Estrella Trujillo | - | Supervisor: Ary Rodriguez |
Name | Thesis | Supervisors |
---|---|---|
Jose Ladino Mendez | Shadows of BH in General Relativity and Alternative Theories | Hernando Quevedo |
Erika Alquicira Peláez | Dynamic and Molecular Evolution of Collimated Outflows in Star-Forming Regions | Ary Rodriguez |
Jesús Carrillo Santamaría | Numerical Simulations of Common Envelopes | Diego Lopez Camara, Fabio De Colle |
José González Carbajal | Evolution and Assembly History of Galaxies Using MHD and Cosmological Simulations | Veronica Lora |
Jorge Osorio Caballero | Galactic Winds Produced by Star Formation Bursts | Ary Rodriguez, Zakaria Meliani (Paris Observatory) |
Karla Vargas Rojas | The Impact of the Progenitor's Stellar Bubble on Its Supernova Remnant | Pablo Velazquez |
Elly Bayona Bobadilla | Gravitational Collapse with Axial Symmetry | Hernando Quevedo |
Antonio Miranda Rosete | False Positives of Biosignatures Generated by a Series of Flares in CO2 Atmospheres of Planets in the Habitable Zone of M Dwarfs | Antigona Segura |
Laura Parrilla de la O | Study of the Nature of the Scalar Field within Horndeski Theories | Tonatiu Matos (CCF), Miguel Alcubierre |
Jorge Castorena Gómez | Study of Knots and Filaments in Planetary Nebulae | Ary Rodriguez, Pedro Rivera Ortiz (IRyA) |
Name | Thesis | Supervisors |
---|---|---|
Diana Páez Sánchez | - | Sarira Sahu, Ary Rodriguez |
Diego Real Arroyo | - | Hernando Quevedo |
José Joaquín Altamirano | - | Miguel Alcubierre |
César Navarrete Zavala | - | Nestor Ortiz |
Jhonnayker Paredes | - | Fabio De Colle |
Ángel Puga Oliveros | - | Sarira Sahu |
Anthony Arenas Martinez | - | Diego Lopez Camara |
At the Instituto de Ciencias Nucleares (ICN), we conduct a wide range of research in astrophysics. Our work explores topics like star formation, high-energy astrophysics, computational astrophysics and data science, and astrobiology. We aim to better understand the universe, from the birth of stars to the conditions that could support life on other planets. The ICN team consists of passionate researchers, students, and postdocs working together to answer some of the biggest questions in science.
We carry out theoretical studies on planetary atmospheres, planetary habitability conditions, and remote detection of life on exoplanets. Additionally, we conduct experimental research on the physical and chemical characteristics of protoplanetary disks and meteorite components.
Researchers: Antígona Segura
We employ high-performance computing to simulate hydrodynamics, magnetohydrodynamics, and radiative transfer in astrophysical phenomenta. Additionally, we apply machine learning and statistical techniques to analyze large astronomical datasets, to understand their behaviour. Also, we develop numerical methods to solve complex astrophysical problems.
Researchers: Fabio De Colle, Diego López-Cámara, Pablo Velázquez
Our research explores the large-scale structure of the Universe, and the nature of dark matter and dark energy.
Researchers: Verónica Lora, Marcelo Salgado
We explore fundamental aspects of strong gravitational fields. In particular, we study the dynamics of compact objects such as neutron stars, black holes, boson stars, and Proca stars, among others.
Researchers: Miguel Alcubierre, Néstor Ortiz, Hernando Quevedo, Marcelo Salgado
Our research focuses on Gamma-Ray Bursts, Supernovae, Tidal Disruption Events, Fast Blue Optical Transients, and other high-energy transients, with an emphasis on using numerical simulations to investigate their complex dynamics. We study the behavior of relativistic jets, shock waves, and the resulting radiation emissions to understand the physical processes driving these events.
Researchers: Fabio De Colle, Diego López-Cámara, Sarira Sahu
Research on star formation focuses on various astrophysical flows, particularly supernova remnants, turbulence in molecular clouds, and protostellar jets. These processes play a crucial role in shaping the interstellar medium and regulating star formation rates. Other studied flows include galactic-scale outflows, such as starburst-driven winds and mass redistribution in galaxies, which influence the long-term evolution of galactic structures. Additionally, researchers investigate photoionized regions and the interaction of exoplanets with stellar winds, providing insights into the conditions that shape planetary atmospheres and their potential habitability.
Researchers: Alejandro Esquivel, Veronica Lora, Ary Rodríguez González, Juan Claudio Toledo Roy, Pablo Velázquez
Our research focuses on stellar evolution of binary systems, particularly the common envelope phase. Using numerical simulations, we study mass transfer, angular momentum dynamics, and their role in forming compact object binaries and producing high energy transitory phenomena.
Researchers: Fabio De Colle, Diego López-Cámara
Students interested in pursuing research in astrophysics can find a variety of thesis topics, both at undergraduate and graduate (master's and PhD) level. We are part of the Graduate Programs in Astrophysics. Some of us are also associated to the Graduate Programs in Earth Science and Physics at UNAM. If you are interested in one of our research topics (see the research section above) feel free to contact us directly.
Postdoctoral positions are available typically every year by an internal competition at UNAM or by using "Conahcyt" funds. Each postdoctoral researcher will have the opportunity to work closely with one of us. Please contact us directly to discuss potential applications.
The Institute of Nuclear Sciences (ICN) at the National Autonomous University of Mexico (UNAM) invites applications for a tenure-track faculty position in the Department of Plasma Physics and Interaction of Radiation with Matter, in one or more of the following research areas:
Application Deadline: April 4, 2025
Minorities and underrepresented groups are especially encouraged to apply.
The initial base salary is set at the standard junior faculty level determined by UNAM ("Investigador Asociado C") and is non-negotiable. For salary inquiries, please contact Dr. Fabio De Colle at fabio@nucleares.unam.mx. Include sriacad@nucleares.unam.mx as cc.
Benefits include:
For further details about the position, application procedure, and required materials, please visit:
Official Job Call (PDF)
To submit your application and provide the contact information for recommendation letters, please apply through:
Online Application Portal
Dr. Fabio De Colle fabio@nucleares.unam.mx. Include sriacad@nucleares.unam.mx as cc.