Astrophysikalisches Seminar

Archiv

  • 21.07.2020, 14:00 Uhr, Prof. Kinwah Wu, MSSL, University College London, UK: tba
  • 18.02.2020, 14:00 Uhr, Mr. Jordy Davelaar, Radboud University Nijmegen, The Netherlands: Particle acceleration in relativistic jets
  • 11.02.2020, 14:00 Uhr, Prof. Dmitri Semikoz, APC Paris: Diffuse TeV gamma-ray emission above 1 TeV
  • 28.01.2020, 14:00 Uhr, Prof. Mark Krumholz, ANU, Australia: Cosmic Rays Across the Star-Forming Galaxy Sequence
  • 10.12.2019, 14:00 Uhr, Dr. Henrike Fleischhack, Michigan Tech University, USA: News from the very-high-energy gamma-ray sky seen by HAWC
  • 12.11.2019, 14:00 Uhr, Dr. Michelle Tsirou, LUPM, Montpellier, France: The morphological asymmetry of very-high-energy gamma-ray pulsar wind nebulae
  • 15.10.2019, 14:00 Uhr, Dr. Damien Bégué, MPE Garching: The problematic connection between gamma-ray bursts and ultra-high energy cosmic rays
  • 02.07.2019, 14:00 Uhr, Prof. Philipp Mertsch, RWTH Aachen: Three elephants in the gamma-ray sky
  • 27.06.2019, 14:00 Uhr, Prof. Yuri Lyubarsky, Ben-Gurion University, Israel: FRB emission mechanisms
  • 15.05.2019, 14:00 Uhr, Dr. Elena Amato, INAF-Arcetri Observatory of Florence, Italy: The physics of Pulsar Wind Nebulae in the light of 3D simulations
  • 30.04.2019, 11:00 Uhr, Dr. Adriano Ingallinera, Univ. Palermo, Italy: Preparing to the ASKAP Galactic science: the SCORPIO project
  • 09.04.2019, 14:00 Uhr, Dr Ellis Owen, MSSL/UCL, Surrey, UK: Star forming galaxies at high redshift in the multi-messenger era
  • 26.03.2019, 14:00 Uhr, Dr. Dmitry Malyshev, FAU Erlangen: Search for the origin of the Fermi bubbles: prospects for H.E.S.S. and CTA
  • 12.03.2019, 14:00 Uhr, Dr. J. Henshaw, MPIA, Heidelberg: The anatomy of the Milky Ways Central Molecular Zone
  • 26.02.2019, 14:00 Uhr, Dr. Luigi Tibaldo, IRAP, Toulouse, France: Future observatories for MeV gamma-ray astronomy
  • 29.01.2019, 14:00 Uhr, Prof. Henrik Beuther, MPI für Astronomie: THOR: The HI/OH/Recombination line survey of the Milky Way
  • 15.01.2019, 14:00 Uhr, Dr. Werner Collmar, MPE, Garching: The MeV-Sky as seen by CGRO/COMPTEL
  • 04.12.2018, 14:00 Uhr, Dr. V. N. Zirakashvili, Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Moscow Troitsk, Russia: Cosmic ray acceleration in accretion flows of galaxy clusters
  • 27.11.2018, 14:00 Uhr, Dr. Oliver Porth, Universität Frankfurt: Pulsar wind nebulae, our relativistic plasma labs in the galaxy
  • 21.09.2018, 11:00 Uhr, Silvia Celli, Gran Sasso Science Institute, L'Aquila, Italy: ACCELERATION, PROPAGATION AND RADIATION OF PARTICLES IN SUPERNOVA REMNANTS WITH CLUMPY STRUCTURE
  • 18.09.2018, 14:00 Uhr, Dr Shinya Nakashima, Riken High Energy Astrophysics Lab, Japan: Hot gas outflows in the Milky Way Galaxy
  • 04.09.2018, 14:00 Uhr, Dr. Roland Crocker, ANU College of Science, Canberra, Australia: Evidence Against a Dark Matter Explanation of the Galactic Centre Excess
  • 20.03.2018, 14:00 Uhr, Rubén López Coto, INFN Padova: Are you living inside a bubble? The answer from nearby pulsars
  • 29.11.2017, 16:30 Uhr, Dr. V.N.Zirakashvili, Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation: Particle acceleration in supernova remnants
  • 22.03.2017, 15:30 Uhr, Dr. Meiert Grootes (ESA/ESTEC): The Effect of group environment on star formation in spiral galaxies
  • 23.09.2016, 11:15 Uhr, Fiona Panther (Research School of Astronomy and Astrophysics, The Australian National University): Galactic positrons from peculiar supernovae
  • 03.02.2016, 15:30 Uhr, Zaza Osmanov, Free University of Tbilisi, Georgia: Centrifugally induced particle acceleration in pulsars and AGNs
  • 20.11.2015, 11:00 Uhr, Prof. Michael Kachelrieß, Norges teknisk-naturvitenskapelige universitet, Trondheim: The escape model for Galactic cosmic rays
  • 04.11.2015, 15:30 Uhr, Dr. Vladimir Zirakashvili, Pushkov Inst. of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Russia: Type IIn supernovae as sources of high energy neutrinos
  • 21.07.2015, 16:00 Uhr, Brenda Dingus, Los Alamos National Lab: HAWC & Beyond: Wide Field of View, Continuous Survey of the TeV Sky
  • 10.06.2015, 11:00 Uhr, Chia-Chun Lu, Taipeh (Taiwan): The high- and low-energy world of the Large Magellanic Cloud
  • 25.02.2015, 15:30 Uhr, Dr. Yuto Teraki, RIKEN, Japan: Particle acceleration in superluminal strong waves
  • 04.02.2015, 15:30 Uhr, Dr. Gwenael Giacinti (Department of Physics, University of Oxford): Particle acceleration at shock break-out
  • 21.01.2015, 15:30 Uhr, Dr. Shuta Tanaka (Institute of Cosmic-Ray Research, University of Tokyo): Pulsar and Magnetar Wind Nebulae
  • 19.01.2015, 15:30 Uhr, Petra Huentemeyer, Michigan Technological University: First Results and Science Potential of the HAWC Observatory
  • 19.11.2014, 15:30 Uhr, Tove Yoast-Hull, Department of Physics, University of Wisconsin-Madison: Cosmic Ray Interactions: Implications for Nearby Starbursts
  • 09.04.2014, 15:30 Uhr, Giovanni Natale, MPIK: 3D ray-tracing radiative transfer in dusty galaxies
  • 07.04.2014, 11:00 Uhr, Dr. Brian Reville, Department of Physics and Astronomy, Queen's University Belfast: Recent developments in cosmic-ray acceleration theory
  • 07.02.2014, 14:00 Uhr, Pol Bordas, MPIK: Discovery of large-scale X-ray jets from the runaway pulsar IGRJ11014-6103
  • 15.01.2014, 15:30 Uhr, Dr. Illya Plotnikov (Institut de Planetologie et d'Astrophysique de Grenoble): PIC simulations of filamentation instabilities in the precursor of relativistic shocks
  • 14.11.2013, 15:30 Uhr, Vladimir N. Zirakashvili (Pushkov Institute for Terrestrial Magnetism, Ionosphere and Radiowave Propagation: Particle acceleration and production of nonthermal emission in supernova remnant Cas A
  • 13.11.2013, 15:30 Uhr, Makoto Takamoto, MPIK: The evolution of high temperature plasma in magnetar magnetospheres and its implications for the Giant Flare
  • 07.08.2013, 15:30 Uhr, Dr. N. Ikhsanov (Pulkovo Observatory, St, Petersburg, Russia): AE Aquarii: a spin-powered pulsar-like white dwarf
  • 31.07.2013, 15:30 Uhr, Amir Levinson, Faculty of Exact Sciences, Tel Aviv University: Radiation mediated shocks and their application to photospheric GRB emission
  • 12.06.2013, 15:30 Uhr, Dr. Roland Crocker, Australian National University: Discovery of Giant Magnetized Lobes Inflated By Galactic Centre Star Formation
  • 29.05.2013, 15:30 Uhr, Dr. Takanobu Amano, Dept. of Earth and Planetary Science, University of Tokyo: The role of superluminal electromagnetic waves in pulsar wind termination shocks
  • 07.02.2013, 15:30 Uhr, Kohta Murase, Institute for Advanced Study, Princeton NJ: Cascade Gamma Rays in the Fermi Era
  • 12.12.2012, 15:30 Uhr, Dr. Tim Cawthorne, Jeremiah Horrocks Institute for Astrophysics and Supercomputing, University of Central Lancashire: What makes jets become bright? Evidence for recollimation shocks in the jets of active galaxies.
  • 17.10.2012, 15:30 Uhr, Iwona Mochol, MPIK: Pulsar Wind Termination Shocks
  • 02.10.2012, 15:30 Uhr, Brian Reville, Clarendon Laboratory, University of Oxford, UK: Laboratory astrophysics using high-power laser produced shocks
  • 12.09.2012, 15:30 Uhr, Makoto Takamoto (MPIK): Enhanced dissipation rate of magnetic field in striped pulsar winds by the effect of turbulence
  • 27.06.2012, 15:30 Uhr, Himadri Ghosh, S. N. Bose National Centre for Basic Sciences, Kolkata, India: Monte Carlo simulations of the advective inflow and outflow around a black hole
  • 10.11.2011, 15:30 Uhr, V. N. Zirakashvili, Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Troitsk:
  • 21.10.2011, 15:30 Uhr, Nigel Maxted, Department of Physics, University of Adelaide: Investigating molecular cores towards the young, gamma-ray-bright supernova remnant RX J1713.7-3946
  • 05.10.2011, 15:30 Uhr, Ioanna Arka, Institut de Planetologie et d'Astrophysique, University of Grenoble: Superluminal waves in pulsar winds: the sigma problem revisited
  • 29.08.2011, 11:00 Uhr, Prof. Don Melrose, School of Physics, University of Sydney: What do plasma astrophysicists ignore by using only half of Maxwell's equations?
  • 18.08.2011, 11:00 Uhr, Dr. Brian Reville, Department of Physics, University of Oxford: Acceleration of cosmic rays and self-generated magnetic turbulence at supernova remnant shocks
  • 20.04.2011, 15:30 Uhr, Dr. Omer Bromberg, Hebrew University, Jerusalem: The propagation of a relativistic jet in an external medium, implication on astrophysical jets and the source of Low luminosity GRBs
  • 09.02.2011, 15:30 Uhr, Dr. Christoph Pfrommer, Heidelberg Institute for Theoretical Studies: Cosmic ray transport in galaxy clusters: implications for radio halos and gamma-rays
  • 16.06.2010, 15:00 Uhr, Dr. Klara Schure, Utrecht University, Netherlands: Time dependent particle acceleration in supernova remnants
  • 21.05.2010, 15:00 Uhr, Dr Markos Georganopoulos, University of Maryland, Baltimore Campus/NASA Goddard: From Blazar Sequence to Blazar Envelope: Unravelling the Fundamental Parameters of Jetted Outflows in Active Galaxies
  • 12.05.2010, 15:00 Uhr, Renzo Capelli, Max-Planck-Institut fuer extraterrestrische Physik, Garching: Fe Ka line emission from Molecular Clouds in the Galactic Center: beyond X-ray Reflection Nebulae
  • 01.04.2010, 15:00 Uhr, Dr. Casey Law, Radio Astronomy Lab, University of California, Berkeley: Probing the Transient Universe with the Allen Telescope Array
  • 17.12.2009, 11:00 Uhr, Vladimir Zirakashvili, Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Russian Academy of Sciences: Cosmic ray acceleration in supernova remnants
  • 16.12.2009, 15:00 Uhr, Mark Dieckmann, Dept. of Science and Technology, Linköping University, Sweden: Particle-in-cell simulation of a mildly relativistic collision of an electron-ion plasma carrying a quasi-parallel magnetic field: Electron acceleration and magnetic field amplification at supernova shocks
  • 11.11.2009, 15:00 Uhr, Joerg Fischera (Canadian Institute for Theoretical Astrophysics): Physical Properties of the coldest regions in the ISM: Condensed Cores
  • 14.10.2009, 15:00 Uhr, Dr. Takanobu Amano (Dept. of Physics, Nagoya University, Japan): A critical Mach number for electron injection in collisionless shocks
  • 19.06.2009, 15:00 Uhr, Anton Dorodnitsyn (NASA Goddard Space Flight Center, Greenbelt, MD, U.S.A.): The formation of narrow X-ray line spectra from realistic hydrodynamical models from warm absorbers to compact object outflows
  • 28.11.2008, 14:00 Uhr, Maxim Barkov (University of Leeds): Very long GRBs
  • 05.11.2008, 15:00 Uhr, Myrto Symeonidis, University College London: (Ultra) Luminous Infrared Galaxies: Their Nature and Evolution
  • 22.10.2008, 15:00 Uhr, Vladimir Zirakashvili (Pushkov Institute of Terrestrial Magnetism, Ionosphere and Radiowave Propagation, Troitsk, Moscow Region, Russia): What are the spectra of particles accelerated in SNRs?
  • 11.06.2008, 15:00 Uhr, R. Belmont (CESR Toulouse): Hot plasma in the Galactic Centre and around accreting black holes
  • 10.06.2008, 15:00 Uhr, Dr. Alexander Konopelko (Purdue University, West Lafayette): VERITAS: Performance and Recent Physics Results
  • 02.06.2008, 15:00 Uhr, Zaza Osmanov (Georgian National Astrophysical Observatory, Tbilisi ): The centrifugally induced curvature drift instability in AGN winds
  • 02.04.2008, 15:00 Uhr, Huirong Yan (Canadian Institute for Theoretical Astrophysics, Toronto): Nonlinear cosmic ray transport and streaming in MHD turbulence
  • 12.03.2008, 15:00 Uhr, Federico Fraschetti (CEA Saclay, France): Ultra-High-Energy Cosmic Rays from the Radio Lobes of AGNs
  • 28.02.2008, 15:00 Uhr, Leonid Ksenofontov (Y. G. Shafer Institute for Cosmophysical Research and Aeronomy, Yakutsk, Russia): Gamma Rays from Tycho's Supernova Remnant
  • 27.02.2008, 15:00 Uhr, Jerome Petri, Centre d'Etudes des Environnements Terrestre et Planetaires, Paris: Modelling the high-energy emission from pulsars