E. van der Swaluw

Bocchino, F., van der Swaluw, E., Chevalier, R., & Bandiera, R. (2005). The nature of the X-ray halo of the plerion G21.5-0.9 unveiled by XMM-Newton and Chandra. Astronomy & Astrophysics, 442, 539-548. https://doi.org/10.1051/0004-6361:20052870 (Original work published 2025)

van der Swaluw, E., Blokland, J. W. S., & Keppens, R. (2005). Convective magneto-rotational instabilities in accretion disks. Astronomy & Astrophysics, 444, 347-355. Retrieved from <Go to ISI>://000233461900010 (Original work published 2025)

Blokland, J. W. S., van der Swaluw, E., Keppens, R., & Goedbloed, J. P. (2005). Magneto-rotational overstability in accretion disks. Astronomy & Astrophysics, 444, 337-346. Retrieved from <Go to ISI>://000233461900009 (Original work published 2025)

van der Swaluw, E. (2005). MHD interaction of pulsar wind nebulae with SNRs and with the ISM. In Young Neutron Stars and Supernova Remnants (Vol. 35, pp. 1123-1128). Retrieved from <Go to ISI>://000231793600025

van der Swaluw, E., & Downes, T. P. (2004). A key to pulsar wind bubble morphologies: Hydrodynamical simulations. In Young Neutron Stars and Their Environments (pp. 175-178). Retrieved from <Go to ISI>://000227426000044

van der Swaluw, E. (2003). Interaction of a magnetized pulsar wind with its surroundings - MHD simulations of pulsar wind nebulae. Astronomy & Astrophysics, 404, 939-947. Retrieved from <Go to ISI>://000183339400015 (Original work published 2025)

van der Swaluw, E., Achterberg, A., Gallant, Y. A., Downes, T. P., & Keppens, R. (2003). Interaction of high-velocity pulsars with supernova remnant shells. Astronomy & Astrophysics, 397, 913-920. Retrieved from <Go to ISI>://000180249800019 (Original work published 2025)