Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Antonis Polatidis"'
Autor:
Jamie McCallum, A. S. Andrianov, J. R. Rizzo, M. S. Burgin, C. García-Miró, Paweł Wolak, E. V. Kravchenko, Yu. A. Kovalev, M. V. Shatskaya, Tuomas Savolainen, James M. Anderson, Alexander B. Pushkarev, A. V. Kovalenko, G. Giovannini, N. N. Shakhvorostova, Marcello Giroletti, A. M. Kutkin, I. A. Rakhimov, Mikhail M. Lisakov, V. I. Kostenko, Norbert Bartel, Sándor Frey, I. N. Pashchenko, Magdalena Kunert-Bajraszewska, Zhi-Qiang Shen, Tapasi Ghosh, D. G. Nair, P. de Vicente, Ivan Litovchenko, Kirill Sokolovsky, J. A. Zensus, Philip G. Edwards, Antonis Polatidis, Shinji Horiuchi, Anastasios Melis, V. A. Zuga, Frank D. Ghigo, Jun Yi Koay, Tao An, P. A. Voitsik, S. F. Likhachev, J. F. H. Quick, I. A. Girin, Marcin P. Gawronski, David L. Jauncey, M. A. Kharinov, C. S. Reynolds, A. E. Melnikov, N. S. Kardashev, Simon Ellingsen, V. Yu. Avdeev, Hayley Bignall, D. V. Ivanov, R. C. Vermeulen, Leonid I. Gurvits, Chris Phillips, Yuri Y. Kovalev, M. A. Shchurov, Alexey Rudnitskiy, Carlo Migoni
Publikováno v:
Advances in Space Research
The largest Key Science Program of the RadioAstron space VLBI mission is a survey of active galactic nuclei (AGN). The main goal of the survey is to measure and study the brightness of AGN cores in order to better understand the physics of their emis
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::772671b24e947bad6776e168efdff4be
https://aaltodoc.aalto.fi/handle/123456789/43103
https://aaltodoc.aalto.fi/handle/123456789/43103
Publikováno v:
Tectonophysics. 367:29-40
Qβ for shear-waves is determined for the inner part of the Hellenic arc, the back-arc area, as a function of frequency in the range 0.6–16 Hz. We used 314 digital records from 32 earthquakes with magnitudes (Mw) ranging from 3.9 to 5.1. Epicentral
Autor:
Antonis Polatidis
Publikováno v:
Proceedings of The 9th European VLBI Network Symposium on The role of VLBI in the Golden Age for Radio Astronomy and EVN Users Meeting — PoS(IX EVN Symposium).
The measurement of expansion velocities in Compact Symmetric Objects, and the calculation of their kinematic ages, showed that the age of these radio sources was of the order of a few hundred to a few thousand years. Further monitoring has proven thi