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Lisa Bugnet's Homepage

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Welcome! I am Lisa Bugnet, an astrophysicist working on the internal dynamics and evolution of stars, using asteroseismology to probe stellar interiors. My research focuses on understanding how physical processes such as internal rotation, magnetic fields, and angular momentum transport affect the evolution of stars, with a particular emphasis on intermediate-mass stars. By interpreting stellar oscillations, I place new constraints on stellar physics that cannot be accessed through surface observations alone.

My ERC Starting Grant project, Calcifer, is dedicated to advancing our understanding of the role of large-scale internal magnetic fields in stellar evolution through magnetoasteroseismology. Recent discoveries have revealed that stable magnetic fields can exist deep within the radiative cores of red giant stars — regions that are hidden from view yet fundamental to a star’s internal dynamics. Traditional stellar evolution models largely neglect these magnetic fields, leading to systematic uncertainties in age estimates and evolutionary pathways for stars like our Sun. By building the first coherent, physically anchored framework for the magnetic evolution of stars, the project aims to revise basic assumptions in stellar physics and improve age diagnostics not only for individual stars but also for stellar populations and galactic archaeology. The funding also supports the growth of a multidisciplinary team covering young stars, evolved giants, and compact remnants, fostering a unified view of magnetism across stellar lifecycles

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​​I began my academic journey with a Ph.D. in Astronomy & Astrophysics from the French Alternative Energies and Atomic Energy Commission (CEA) and Paris-Cité University in 2020, where I focused on stellar structure and dynamics through asteroseismology. I was a Flatiron Research Fellow at the Center for Computational Astrophysics of the Flatiron Institute in New York (2020–2022). In 2023, I joined the Institute of Science and Technology Austria (ISTA) as the first Assistant Professor in Astronomy, where I established the Asterics research group. I am Associate Editor for Astronomy & Astrophysics since January 2026.

14. Jän. 2026

Near-degeneracy effects in Quadrupolar Mixed Modes. From an Asymptotic Description to Data Fitting.

Accepted for publication in A&A

2. Juli 2025

Exploring the probing power of γ-Dor’s inertial dip
for core magnetism: case of a toroidal field

Accepted for publication in A&A

9. Dez. 2024

Constraining differential rotation in gamma Doradus stars from inertial dips properties

Accepted for Publication in A&A

31. Mai 2024

Unveiling complex magnetic field configurations in red giant stars

Published in A&A

29. Apr. 2024

Detectability of axisymmetric magnetic fields from the core to the surface of oscillating post-main sequence stars

Published in ApJ

16. Nov. 2022

Mode Mixing and Rotational Splittings. I. Near-degeneracy Effects Revisited

1. Aug. 2023

Magnetic Activity Evolution of Solar-like Stars. I. S ph-Age Relation Derived from Kepler Observations

24. Aug. 2022

Magnetic signatures on mixed-mode frequencies

II. Period spacings as a probe of the internal magnetism of red giants

11. Juni 2023

Asymmetries of frequency splittings of dipolar mixed modes: a window on the topology of deep magnetic fields

©2026 by Asterics @ ISTA

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