Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Pohl, Martin Karl Wilhelm (Prof. Dr.)"'
Autor:
Bohdan, Artem, Niemiec, Jacek, Pohl, Martin Karl Wilhelm (Prof. Dr.), Matsumoto, Yosuke, Amano, Takanobu, Hoshino, Masahiro
Electron injection at high Mach number nonrelativistic perpendicular shocks is studied here for parameters that are applicable to young SNR shocks. Using high-resolution large-scale two-dimensional fully kinetic particle-in-cell simulations and traci
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______266::1668232dcfe446818cf8fc6de25a43eb
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/49058
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/49058
Autor:
Petruk, Oleh, Kuzyo, T., Orlando, S., Pohl, Martin Karl Wilhelm (Prof. Dr.), Miceli, M., Bocchino, F., Beshley, V., Brose, Robert (Dr.)
We present very-high-resolution 1D MHD simulations of the late-stage supernova remnants (SNRs). In the post-adiabatic stage, the magnetic field has an important and significant dynamical effect on the shock dynamics, the flow structure, and hence the
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______266::74aa6e6ec326b4747057166240ab2c2e
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/52125
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/52125
X-RAY OBSERVATIONS OF BOW SHOCKS AROUND RUNAWAY O STARS. THE CASE OF zeta OPH AND BD+43 degrees 3654
Autor:
Toala, J. A., Oskinova, Lida M., Gonzalez-Galan, Ana, Guerrero, M. A., Ignace, R., Pohl, Martin Karl Wilhelm (Prof. Dr.)
Non-thermal radiation has been predicted within bow shocks around runaway stars by recent theoretical works. We present X-ray observations toward the runaway stars zeta Oph by Chandra and Suzaku and of BD+43 degrees 3654 by XMM-Newton to search for t
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______266::c805a2b8a0c958ca6c4334979693c9a4
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/45423
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/45423
Autor:
Archambault, S., Archer, A., Aune, T., Barnacka, Anna, Benbow, W., Bird, R., Buchovecky, M., Buckley, J. H., Bugaev, V., Byrum, K., Cardenzana, J. V., Cerruti, M., Chen, Xuhui, Ciupik, L., Collins-Hughes, E., Connolly, M. P., Cui, W., Dickinson, H. J., Dumm, J., Eisch, J. D., Falcone, A., Feng, Q., Finley, J. P., Fleischhack, H., Flinders, A., Fortin, P., Fortson, L., Furniss, A., Gillanders, G. H., Griffin, S., Grube, J., Gyuk, G., Huetten, M., Hakansson, Nils, Hanna, D., Holder, J., Humensky, T. B., Johnson, C. A., Kaaret, P., Kar, P., Kelley-Hoskins, N., Kertzman, M., Khassen, Y., Kieda, D., Krause, M., Krennrich, F., Kumar, S., Lang, M. J., Maier, G., McArthur, S., McCann, A., Meagher, K., Millis, J., Moriarty, P., Mukherjee, R., Nieto, D., Ong, R. A., Otte, A. N., Pandel, D., Park, N., Pelassa, V., Pohl, Martin Karl Wilhelm (Prof. Dr.), Popkow, A., Pueschel, Elisa, Quinn, J., Ragan, K., Reynolds, P. T., Richards, G. T., Roache, E., Rousselle, J., Rulten, C., Santander, M., Sembroski, G. H., Shahinyan, K., Smith, A. W., Staszak, D., Telezhinsky, Igor O., Tucci, J. V., Tyler, J., Vincent, S., Wakely, S. P., Weiner, O. M., Weinstein, A., Wilhelm, Alina, Williams, D. A., Zitzer, B.
The TeV binary system LS I +61 degrees 303 is known for its regular, non-thermal emission pattern that traces the orbital period of the compact object in its 26.5 day orbit around its B0 Ve star companion. The system typically presents elevated TeV e
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=od_______266::6147feb28e37749d1dc916aa810e1927
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/45685
https://publishup.uni-potsdam.de/frontdoor/index/index/docId/45685