Postdoc in Stellar Astrophysics

This project explores the effects of magnetic fields on stellar structure and mixing processes within stars. It focuses on magnetic field generation, the impact on pulsations, and broader implications for stellar evolution. MAGNIFY investigates the variability induced by stellar spots and examines the origin of magnetic fields causing these variations in A and F stars. Using asteroseismology, we aim to detect and analyze near-core and surface magnetic fields. This involves comparing theoretical models with photometric observations from the Kepler and TESS satellites, complemented by Gaia data and ground-based spectroscopic and spectropolarimetric observations.

Responsibilities
As a Postdoctoral Researcher, you will among other:

• Create and coordinate a comprehensive grid of stellar and pulsation models for A and F stars.
• Analyze how different model parameters affect pulsation characteristics.
• Use asteroseismology to study near-core and surface magnetic fields, integrating findings into a broader understanding of stellar structures.
• Analyze how magnetic fields affect pulsation frequencies 
• Publish findings in scientific journals and present at research seminars and conferences.
• Mentor and support students and PhD students engaged in related research activities.
• Promote equity and diversity within the research team, fostering an inclusive and collaborative work environment.

Qualifications

• Extensive experience in stellar modeling 
• Experience in magneto-asteroseismology is highly desirable.
• Strong analytical skills and a proven track record of research publications.
• Proven ability to conduct independent research
• Effective communication and mentoring skills.
• A commitment to diversity and inclusion in the workplace.

Application procedure 
Your complete online application must be submitted no later than 15 September 2024 (23:59 Danish time). 

To view the full announcement and to apply: Postdoc in Stellar Astrophysics