Zobrazeno 1 - 3
of 3
pro vyhledávání: '"Ann-Sofie Bak Nielsen"'
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
Autor:
Ziwei Wu, Joris P. W. Verbiest, Robert A. Main, Jean-Mathias Grießmeier, Yulan Liu, Stefan Osłowski, Krishnakumar Moochickal Ambalappat, Ann-Sofie Bak Nielsen, Jörn Künsemöller, Julian Y. Donner, Caterina Tiburzi, Nataliya Porayko, Maciej Serylak, Lars Künkel, Marcus Brüggen, Christian Vocks
Context. Interstellar scintillation (ISS) of pulsar emission can be used both as a probe of the ionised interstellar medium (IISM) and cause corruptions in pulsar timing experiments. Of particular interest are so-called scintillation arcs which can b
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::45a551f1219e62ab0131f998abda4782
http://arxiv.org/abs/2203.10409
http://arxiv.org/abs/2203.10409
Publikováno v:
Astronomy and Astrophysics, 611, A67
The physical characteristics of dust formed in supernovae is poorly known. In this paper, we investigate the extinction properties of dust formed in the type IIn SN 2005ip. The observed light curves of SN 2005ip all exhibit a sudden drop around 50 da
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::672192fadcfc4c039563ef75ebfc8c22
http://hdl.handle.net/1887/69552
http://hdl.handle.net/1887/69552