Intra cluster MAGnetic fields origiNATing from star formatION processes

• Applicant: Professor Dr. Klaus Dolag
• Subject Area: Astrophysics and Astronomy
• Term: from 2009 to 2012
• Project identifier: Deutsche Forschungsgemeinschaft (DFG) - Project number 126995580

• Final Report Year: 2012

Final Report Abstract

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.

Publications

• (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.
  (See online at 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.
  (See online at 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.
  (See online at 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.
  (See online at 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.
  (See online at https://doi.org/10.1111/j.1365-2966.2011.18932.x)