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Magnetic field in a turbulent galactic diskOTMIANOWSKA-MAZUR, K.Symposium - International astronomical union. 1989, Num 140, pp 157-158, issn 0074-1809, 2 p.Conference Paper

Dynamo coefficients in Parker unstable disks with cosmic rays and shear : The new methods of estimationKOWAL, G; OTMIANOWSKA-MAZUR, K; HANASZ, M et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 445, Num 3, pp 915-929, issn 0004-6361, 15 p.Article

Magnetic field in a turbulent galactic diskOTMIANOWSKA-MAZUR, K; URBANIK, M; TERECH, A et al.Geophysical and astrophysical fluid dynamics. 1992, Vol 66, Num 1-4, pp 209-222, issn 0309-1929Article

NUMERICAL TESTS OF FAST RECONNECTION IN WEAKLY STOCHASTIC MAGNETIC FIELDSKOWAL, Grzegorz; LAZARIAN, A; VISHNIAC, E. T et al.The Astrophysical journal. 2009, Vol 700, Num 1, pp 63-85, issn 0004-637X, 23 p., 1Article

GLOBAL SIMULATIONS OF THE MAGNETIC FIELD EVOLUTION IN BARRED GALAXIES UNDER THE INFLUENCE OF THE COSMIC-RAY-DRIVEN DYNAMOKULPA-DYBEL, K; OTMIANOWSKA-MAZUR, K; KULESZA-ZYDZIK, B et al.The Astrophysical journal. 2011, Vol 733, Num 2, issn 0004-637X, 733l18.1-733L18.6, 2Article

The influence of the cluster environment on the large-scale radio continuum emission of 8 Virgo cluster spiralsVOLLMER, B; SOIDA, M; CHUNG, A et al.Astronomy and astrophysics (Berlin. Print). 2010, Vol 512, issn 0004-6361, 512A36.1-512A36.15Article

A dynamical model for the heavily ram pressure stripped Virgo spiral galaxy NGC 4522VOLLMER, B; SOIDA, M; OTMIANOWSKA-MAZUR, K et al.Astronomy and astrophysics (Berlin. Print). 2006, Vol 453, Num 3, pp 883-893, issn 0004-6361, 11 p.Article

The characteristic polarized radio continuum distribution of cluster spiral galaxiesVOLLMER, B; SOIDA, M; BECK, R et al.Astronomy and astrophysics (Berlin. Print). 2007, Vol 464, Num 3, issn 0004-6361, L37-L40Article

Pre-peak ram pressure stripping in the Virgo cluster spiral galaxy NGC 4501VOLLMER, B; SOIDA, M; CHUNG, A et al.Astronomy and astrophysics (Berlin. Print). 2008, Vol 483, Num 1, pp 89-106, issn 0004-6361, 18 p.Article

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