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pro vyhledávání: '"Olexandr O Konovalenko"'
Autor:
Ziwei Wu, William A Coles, Joris P W Verbiest, Krishnakumar Moochickal Ambalappat, Caterina Tiburzi, Jean-Mathias Grießmeier, Robert A Main, Yulan Liu, Michael Kramer, Olaf Wucknitz, Nataliya Porayko, Stefan Osłowski, Ann-Sofie Bak Nielsen, Julian Y Donner, Matthias Hoeft, Marcus Brüggen, Christian Vocks, Ralf-Jürgen Dettmar, Gilles Theureau, Maciej Serylak, Vladislav Kondratiev, James W McKee, Golam M Shaifullah, Ihor P Kravtsov, Vyacheslav V Zakharenko, Oleg Ulyanov, Olexandr O Konovalenko, Philippe Zarka, Baptiste Cecconi, Léon V E Koopmans, Stéphane Corbel
Publikováno v:
Mon.Not.Roy.Astron.Soc.
Mon.Not.Roy.Astron.Soc., 2023, 520 (4), pp.5536-5543. ⟨10.1093/mnras/stad429⟩
Mon.Not.Roy.Astron.Soc., 2023, 520 (4), pp.5536-5543. ⟨10.1093/mnras/stad429⟩
Interstellar scattering (ISS) of radio pulsar emission can be used as a probe of the ionised interstellar medium (IISM) and causes corruptions in pulsar timing experiments. Two types of ISS phenomena (intensity scintillation and pulse broadening) are
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::83704b5ff24d4703ff540ef1e7746c8f
https://doi.org/10.1093/mnras/stad429
https://doi.org/10.1093/mnras/stad429