Seminars

The AI Revolution in Academia: A Practical & Honest Guide for Researchers and Teachers
Maxime Fays (ULiege - STAR - Ograv)

Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)

Ready or not, Generative AI is reshaping how research is done and how students learn. This talk cuts through the noise with practical techniques and honest assessments of both the potential and the pitfalls: what these tools actually are, where they reliably fail, and how to direct them effectively whether for writing grants, designing exams, or reclaiming time spent on tasks AI handles in seconds.

Comet C/2020 F3 (NEOWISE): From naked eye spectacle to scientific insights
Aravind Krishnakumar (STAR Institute Université de Liège)

Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)

Comets are among the most primitive bodies in the Solar System, preserving a record of the physical and chemical conditions prevalent during their formation. The study of cometary comae through photometry and spectroscopy provides critical insights into volatile composition and outgassing processes. In particular, production rates of commonly observed species such as OH, NH, CN, C₂, and C₃ serve as key diagnostics of the nucleus composition and its evolutionary state. The abundance of molecular nitrogen relative to CO and H₂O, however, remains poorly constrained. In the optical regime, these parent volatiles can be probed only indirectly through their ionic emissions, making their detection both essential and challenging due to their extremely low densities. The Great Comet of 2020, C/2020 F3 (NEOWISE), has been extensively studied using very high-resolution spectroscopy; however, ionic emissions have not been previously reported. In contrast, long-slit low-resolution spectroscopy of such a bright comet enables detailed investigation of spatial emission profiles, offering a complementary and powerful diagnostic. In this seminar, I will take you through the realm of cometary science and present the detection of ionic emissions, including N₂⁺, CO⁺, and H₂O⁺ in C/2020 F3 (NEOWISE), along with other unusual spectral features. I will discuss the derived relative abundances and their implications for cometary formation conditions and volatile chemistry, alongside an overview of production rates of key neutral species. Additionally, I will highlight the detection of a particularly intriguing optical emission and explore its potential significance.

TBD
Angelos Nersesian (STAR Institute Université de Liège)

Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)

TBD

Genesis: the ESA mission to measure Earth down to the millimeter
Gilles Wautelet (LPAP, STAR Institute, ULiège)

Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)

TBD

TBD
Martin Farnir (STAR Institute Université de Liège)

Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)

TBD

Orion’s Massive Stars: Delta and Epsilon Ori
Alžběta Oplištilová (STAR Institute Université de Liège)

Salle de réunion AGO (local -1/14), Institut d'Astrophysique et de Géophysique
Bâtiment B5c, Quartier Agora, Allée du 6 Août, 19C, B-4000 Liège 1 (Sart-Tilman)

Massive stars are cosmic engines. By exploding as supernovae, they power galaxies, shape the interstellar medium, and enrich it with heavy elements. Yet, their inner workings remain among the most challenging frontiers in stellar astrophysics. The evolution of massive stars is critically influenced by multiplicity; most have one or more companions, while a few remain single. This raises the question: could these single stars be the end products of multiple systems? Interferometry is one of the best methods for detecting and characterising stellar multiplicity. The Orion complex is the nearest massive-star-forming region with multiple OB stars, and thus the most suitable for detailed studies. It hosts a number of massive stars, particularly in the Orion Belt. I constructed two complex models: the triple star Delta Ori and the single star Epsilon Ori using interferometric data in synergy with astrometry, photometry, high-resolution spectroscopy, and spectral energy distribution. Delta Ori is currently in the pre-mass-transfer evolutionary stage, while Epsilon Ori is a significantly oblate supergiant due to its rapid rotation. As the only massive single star in the Orion Belt, Epsilon Ori likely follows a non-standard evolutionary path.