Work emails | zajacek@mail.muni.cz
zajacek@cft.edu.pl zajacek@ph1.uni-koeln.de |
Website | physics.muni.cz/~zajacek/ |
Office address | Department of Theoretical Physics and Astrophysics, Kotlářská 2, 602 00, Brno, Czech Republic |
10/2017 | PhD in Astrophysics “Interplay between interstellar medium and black hole environment” at the University of Cologne and Max Planck Institute for Radioastronomy, Germany; PhD advisors: Prof. Dr. Andreas Eckart & Prof. Dr. Anton Zensus |
12/2014 | Rigorosum examination (RNDr. title) Charles University in Prague |
06/2014 | MSc in Astronomy & Astrophysics “Neutron stars near a galactic center” at the Charles University in Prague; Supervisor: Prof. Dr. Vladimír Karas |
06/2012 | BSc in General Physics “The Late Heavy Bombardment at various places of the Solar System” at the Charles University in Prague; Supervisor: Assoc. Prof. Dr. Miroslav Brož |
since 2021 | Postdoctoral researcher in the High-Energy Astrophysics group, Department of Theoretical Physics and Astrophysics at the Masaryk University, Brno, Czech Republic |
2019-2021 | Postdoctoral researcher in the Center for Theoretical Physics (quasar group of Prof. B. Czerny), Polish Academy of Sciences, Warsaw, Poland |
2017-2019 | Junior postdoctoral fellow in the Very Long Baseline Interferometry group, Max Planck Institute for Radioastronomy, Bonn, Germany |
Michal is a postdoctoral researcher in the High-Energy Astrophysics group at the Department of Theoretical Physics and Astrophysics, Masaryk University in Brno, Czechia. He has been studying a broad range of phenomena in galactic nuclei, including star-formation in the Galactic center, broad-line region dynamics in active galactic nuclei as well as kinematics of jets in blazars. In recent years, he has also become interested in the application of quasars for constraining cosmological parameters.
Michal did his PhD degree at the University of Cologne within the framework of the International Max Planck Research School (IMPRS) for Astronomy & Astrophysics in 2017. He has been working on the dynamics of gas and stars in the vicinity of a supermassive black hole, with the application to interpret the near-infrared observations of the Galactic Center. He also dedicated a part of his PhD for studying radio-optical properties of a sample of intermediate-redshift galaxies. Later, for one year and a few months, he continued at the MPIfR in Bonn to study the signs of jet precession in radio galaxies. Later, during his postdoctoral stay in Warsaw, Poland, he dedicated a significant part of his research to the reverberation-mapping of luminous, higher-redshift quasars using broad MgII and FeII lines. Among his most important reseach contributions are the confirmation of MgII radius-luminosity relation and its application to cosmology, the tentative confirmation of pre-main-sequence stars around Sgr A* on the scale of 10000 AU from the supermassive black hole, the explanation of the lack of large red giants in the Galactic center, the methodology for constraining electric charge of Sgr A*, and the application of the jet precession model to interpret the variability of some radio galaxies.
In his free time, Michal is involved in the public outreach of astronomy results. In addition, he is dedicated to the informal education of elementary and high-school students. He collaborates with the non-profit organization AMAVET (Association for Youth, Science, and Technology). He also established a multidisciplinary online seminar LaBaK, which is intended for kindergarten children, elementary, and high-school students.
For a complete list of publications see here.
High Energy Astrophysics Group
Department of Theoretical Physics and Astrophysics
Kotlářská 2, 602 00, Brno
Czech Republic