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Devika Tharakkal, Anvar Shukurov, Frederick A Gent, Graeme R Sarson, Andrew P Snodin and Luiz Felippe S Rodrigues Monthly Notices of the Royal Astronomical Society 525(4) 5597 (2023) https://doi.org/10.1093/mnras/stad2610
Non-linear magnetic buoyancy instability and turbulent dynamo
Yasin Qazi, Anvar Shukurov, Devika Tharakkal, Frederick A Gent and Abhijit B Bendre Monthly Notices of the Royal Astronomical Society 527(3) 7994 (2023) https://doi.org/10.1093/mnras/stad3684
Chandra large-scale mapping of the Galactic Centre: probing high-energy structures around the central molecular zone
Similarity between the Molecular Loops in the Galactic Center and the Solar Chromospheric Arch Filaments
Kunio Takahashi, Satoshi Nozawa, Ryoji Matsumoto, Mami Machida, Yasuo Fukui, Natsuko Kudo, Kazufumi Torii, Hiroaki Yamamoto and Motosuji Fujishita Publications of the Astronomical Society of Japan 61(5) 957 (2009) https://doi.org/10.1093/pasj/61.5.957
Cosmic-ray driven dynamo in galactic disks
Michał Hanasz, K. Otmianowska-Mazur, H. Lesch, et al. Proceedings of the International Astronomical Union 4(S259) 479 (2009) https://doi.org/10.1017/S1743921309031147
CAN THE COSMIC RAY DRIVEN DYNAMO MODEL EXPLAIN THE OBSERVATIONS OF THE POLARIZED EMISSION OF EDGE-ON GALAXIES?
Katarzyna Otmianowska-Mazur, Marian Soida, Barbara Kulesza-Żydzik, Michał Hanasz and Grzegorz Kowal The Astrophysical Journal 693(1) 1 (2009) https://doi.org/10.1088/0004-637X/693/1/1
K. Otmianowska-Mazur, M. Hanasz and G. Kowal Astrophysics and Space Science Library, How does the Galaxy Work? 315 303 (2005) https://doi.org/10.1007/1-4020-2620-X_61
Global dynamical evolution of the ISM in star forming galaxies
Magnetic Reconnection Triggered by the Parker Instability in the Galaxy: Two‐dimensional Numerical Magnetohydrodynamic Simulations and Application to the Origin of X‐Ray Gas in the Galactic Halo
Syuniti Tanuma, Takaaki Yokoyama, Takahiro Kudoh and Kazunari Shibata The Astrophysical Journal 582(1) 215 (2003) https://doi.org/10.1086/344523
Incorporation of cosmic ray transport into the ZEUS MHD code