Πρόσφατες δημοσιεύσεις των μελών της ομάδας μας:

  1. Axisymmetric magneto-plastic evolution of neutron-star crusts, K.N. Gourgouliatos, S.K. Lander, MNRAS, 506, 3, pp.3578-3587, 2021.
  2. Polytropic wind solutions via the Complex Plane Strategy, V. Karageorgopoulos, K.N. Gourgouliatos, V. Geroyannis, Astronomy and Computing, Volume 36, article id. 100491, 2021
  3. Magnetic Inhibition of the Recollimation Instability in Relativistic Jets, J. Matsumoto, S.S. Komissarov, K.N. Gourgouliatos, MNRAS, 503, 4, pp.4918-4929, 2021
  4. 3D Magnetothermal Simulations of Tangled Crustal Magnetic Field in Central Compact Objects, ApJ, A. Igoshev, K.N. Gourgouliatos, R. Hollerbach, T. Wood, 909, 2, 101, 9 pp., 2021
  5. Sensitivity of the Cherenkov Telescope Array for probing cosmology and fundamental physics with gamma-ray propagation, H. Abdalla et al., Journal of Cosmology and Astroparticle Physics, Issue 02, article id. 048, 2021.
  6. Sensitivity of the Cherenkov Telescope Array to a dark matter signal from the Galactic centre, Acharrya A. et al., 2021, Journal of Cosmology and Astroparticle Physics, 01, 057.
  7. Strong toroidal magnetic fields required by quiescent X-ray emission of magnetars, Igoshev A., Hollerbach R., Wood T., Gourgouliatos K.N., Nature Astronomy, 215, 2021.
  8. Three-dimensional Modeling of the Magnetothermal Evolution of Neutron Stars: Method and Test Cases, De Grandis D., Turolla R., Wood T.S., Zane S., Taverna R., Gourgouliatos, K.N., 2020, ApJ 903, 40.
  9. Powering central compact objects with a tangled crustal magnetic field; Gourgouliatos K.N., Hollerbach R., Igoshev A., MNRAS, 2020, 495, 1692.
  10. Obscuration properties of mid-IR-selected AGN; Mountrichas, G., Georgantopoulos, I., Ruiz, A., Kampylis, G., MNRAS, 2020, 491, 1727.
  11. Nonaxisymmetric Hall instability: A key to understanding magnetars; Gourgouliatos K.N., Pons J., Phys.Rev.Research, 2019, 1,032049.
  12. Current closure through the neutron star crust; Karegorgopoulos V., Gourgouliatos K.N., Contopoulos I., MNRAS, 2019, 487, 3333.