Research Center for Astronomy

Events

Tuesday 8 April 2025, 12:00

WEBINAR

A JWST investigation into barred galaxies at high redshifts z > 1

Zoe A. Le Conte

Department of Physics, Durham University

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Featured Picture

Pulsar Magnetosphere with Machine Learning

 

Cross section of the steady-state ideal force-free pulsar magnetosphere for an inclined dipole rotator. Rotation axis along z. Thick black lines: separatrix between open and closed field lines. The color scale represents the development of the azimuthal magnetic field Bφ due to the pulsar rotation. Υellow: no Bφ. Dark purple: only Bφ. (from Dimitropoulos, Chaniadakis & Contopoulos 2025, submitted to Astronomy & Astrophysics, arXiv:2410.10716v2)


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The Annual Report of our Center for 2024 is available in Greek  and in English

               

 

 

RCAAM presentation at the one-day workshop on February 19th 2024 at the central building of the Academy of Athens


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