Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Vlahakis, N."'
Autor:
Rani, B., Petropoulou, M., Zhang, H., D'Ammando, F., Finke, J., Baring, M., Böttcher, M., Dimitrakoudis, S., Gan, Z., Giannios, D., Hartmann, D. H., Krichbaum, T. P., Marscher, A. P., Mastichiadis, A., Nalewajko, K., Ojha, R., Paneque, D., Shrader, C., Sironi, L., Tchekhovskoy, A., Thompson, D. J., Vlahakis, N., Venters, T. M.
Active galactic nuclei (AGN) with relativistic jets, powered by gas accretion onto their central supermassive black hole (SMBH), are unique laboratories for studying the physics of matter and elementary particles in extreme conditions that cannot be
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a8abb952cc62b69b537a2fff0420a3ed
Autor:
Matsakos, T., Vlahakis, N., Tsinganos, K., Karampelas, K., Sauty, C., Cayatte, V., Matt, S. P., Massaglia, S., Trussoni, E., Mignone, A.
It is a well established fact that some YSO jets (e.g. RW Aur) display different propagation speeds between their blue and red shifted parts, a feature possibly associated with the central engine or the environment in which the jet propagates. In ord
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a001455f0a5d4393d689a667b2e12bb1
We present numerical simulations of axisymmetric, magnetically driven relativistic jets. To eliminate the dissipative effects induced by a free boundary with an ambient medium we assume that the flow is confined by a rigid wall of a prescribed shape,
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::ef216b51ae8d7fdbe1ad7c34d3de6404
The classical Blandford & Payne (1982) model for the magnetocentrifugal acceleration and collimation of a disk-wind is revisited and refined. In the original model, the gas is cold and the solution is everywhere subfast magnetosonic. In the present m
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::227b0dac116f0a3155f90072626b56a5
Autor:
Vlahakis, N., Tsinganos, K.
By a systematic method we construct general classes of exact and selfconsistent axisymmetric MHD solutions describing flows which originate at the near environment of a central gravitating astrophysical object. The unifying scheme contains two large
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::9afa6f74ffb04142daded291d94c5a14
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