Intra cluster MAGnetic fields origiNATing from star formatION processes

• Antragsteller: Professor Dr. Klaus Dolag
• Fachliche Zuordnung: Astrophysik und Astronomie
• Förderung: Förderung von 2009 bis 2012
• Projektkennung: Deutsche Forschungsgemeinschaft (DFG) - Projektnummer 126995580

• Erstellungsjahr: 2012

Zusammenfassung der Projektergebnisse

Galaxy clusters are the largest, quasi-equilibrium objects in the Universe, making them extraordinarily interesting for cosmology and astrophysics. In these systems, non-thermal components such as magnetic field and high energy particles keep a record of the processes acting since early times till now. These components play key roles by controlling transport processes inside the cluster atmosphere and are sources of additional pressure and energy support. The evolution and the structure of magnetic fields can be explored and within fully self consistent, cosmological MHD simulations. The resulting magnetization of the ICM will is the compared with recent observations in radio band. The inferred magnetization of the large scale structure of the universe is compared with recent findings of the propagation of high energy cosmic messenger particles.

Projektbezogene Publikationen (Auswahl)

• (2010). Measuring cosmic magnetic fields by rotation measure–galaxy cross-correlations in cosmological simulations. Monthly Notices of the Royal Astronomical Society, 408(2), 684-694
  Stasyszyn, F., Nuza, S. E., Dolag, K., Beck, R., Donnert, J.
  (Siehe online unter https://doi.org/10.1111/j.1365-2966.2010.17166.x)
• (2010). Rotation measures of radio sources in hot galaxy clusters. Astronomy & Astrophysics, 522, A105
  Govoni, F., Dolag, K., Murgia, M., Feretti, L., Schindler, S., Giovannini, G., Boschin, W., Vacca, V., Bonafede, A.
  (Siehe online unter https://doi.org/10.1051/0004-6361/200913665)
• (2010): Radio haloes from simulations and hadronic models – I. The Coma cluster. In: Mon Not R Astron Soc 401 (1), S. 47–54
  Donnert, J., Dolag, K., Cassano, R., Brunetti, G.
  (Siehe online unter https://doi.org/10.1111/j.1365-2966.2009.15655.x)
• (2011). A non-ideal magnetohydrodynamic GADGET: simulating massive galaxy clusters. Monthly Notices of the Royal Astronomical Society, 418(4), 2234-2250
  Bonafede, A., Dolag, K., Stasyszyn, F., Murante, G., Borgani, S.
  (Siehe online unter https://doi.org/10.1111/j.1365-2966.2011.19523.x)
• (2011). Galactic ménage à trois: simulating magnetic fields in colliding galaxies. Monthly Notices of the Royal Astronomical Society, 415(4), 3189-3218
  Kotarba, H., Lesch, H., Dolag, K., Naab, T., Johansson, P. H., Donnert, J., Stasyszyn, F. A.
  (Siehe online unter https://doi.org/10.1111/j.1365-2966.2011.18932.x)