Zobrazeno 1 - 10
of 93
pro vyhledávání: '"V. Heesen"'
Autor:
V. Heesen, S. P. O’Sullivan, M. Brüggen, A. Basu, R. Beck, A. Seta, E. Carretti, M. G. H. Krause, M. Haverkorn, S. Hutschenreuter, A. Bracco, M. Stein, D. J. Bomans, R.-J. Dettmar, K. T. Chyży, G. H. Heald, R. Paladino, C. Horellou
Publikováno v:
Astronomy & Astrophysics, 670, pp. 1-5
Astronomy & Astrophysics, 670, 1-5
Astronomy & Astrophysics, 670, 1-5
Context. The existence of magnetic fields in the circumgalactic medium (CGM) is largely unconstrained. Their detection is important as magnetic fields can have a significant impact on the evolution of the CGM and, in turn, the fields can serve as tra
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::0fe40abcc103b3cabb857ac9bf79dd0c
https://repository.ubn.ru.nl/handle/2066/290178
https://repository.ubn.ru.nl/handle/2066/290178
Autor:
S P O’Sullivan, T W Shimwell, M J Hardcastle, C Tasse, G Heald, E Carretti, M Brüggen, V Vacca, C Sobey, C L Van Eck, C Horellou, R Beck, M Bilicki, S Bourke, A Botteon, J H Croston, A Drabent, K Duncan, V Heesen, S Ideguchi, M Kirwan, L Lawlor, B Mingo, B Nikiel-Wroczyński, J Piotrowska, A M M Scaife, R J van Weeren
A Faraday rotation measure (RM) catalogue, or RM Grid, is a valuable resource for the study of cosmic magnetism. Using the second data release (DR2) from the LOFAR Two-metre Sky Survey (LoTSS), we have produced a catalogue of 2461 extragalactic high-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::162a3e0ba9936f99d92b996598175a09
Autor:
L. Gajović, F. Welzmüller, V. Heesen, F. de Gasperin, M. Vollmann, M. Brüggen, A. Basu, R. Beck, D. J. Schwarz, D. J. Bomans, A. Drabent
Weakly interacting massive particles (WIMPs) can self-annihilate, thus providing us with a way to indirectly detect dark matter (DM). Dwarf spheroidal (dSph) galaxies are excellent places to search for annihilation signals because they are rich in DM
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::3fdbf0084daad0475025509620f128c5
https://doi.org/10.1051/0004-6361/202245508
https://doi.org/10.1051/0004-6361/202245508
Akademický článek
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Autor:
V. Heesen, F. de Gasperin, S. Schulz, A. Basu, R. Beck, M. Brüggen, R.-J. Dettmar, M. Stein, L. Gajović, F. S. Tabatabaei, P. Reichherzer
Publikováno v:
Astronomy & Astrophysics. 672:A21
Context. The details of cosmic-ray transport have a strong impact on galaxy evolution. The peak of the cosmic-ray energy distribution is observable in the radio continuum using the electrons as proxy. Aims. We measure the length that the cosmic-ray e
Autor:
M. Stein, V. Heesen, R.-J. Dettmar, Y. Stein, M. Brüggen, R. Beck, B. Adebahr, T. Wiegert, C. J. Vargas, D. J. Bomans, J. Li, J. English, K. T. Chyży, R. Paladino, F. S. Tabatabaei, A. Strong
Publikováno v:
Astronomy & Astrophysics. 670:A158
Galactic winds play a key role in regulating the evolution of galaxies over cosmic time. In recent years, the role of cosmic rays (CR) in the formation of the galactic wind has increasingly gained attention. Therefore, we use radio continuum data to
Autor:
V. Heesen, T.-L. Klocke, M. Brüggen, F. S. Tabatabaei, A. Basu, R. Beck, A. Drabent, B. Nikiel-Wroczyński, R. Paladino, S. Schulz, M. Stein
Context. Magnetic fields are key to understand galaxy evolution, regulating stellar feedback and star formation in galaxies. Aims. We probe the origin of magnetic fields in late-type galaxies, measuring magnetic field strengths, exploring whether mag
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::bb40f83ce9f219206bd99ba0c31eff8e
Autor:
V. Heesen, M. Staffehl, A. Basu, R. Beck, M. Stein, F. S. Tabatabaei, M. J. Hardcastle, K. T. Chyży, T. W. Shimwell, B. Adebahr, R. Beswick, D. J. Bomans, A. Botteon, E. Brinks, M. Brüggen, R.-J. Dettmar, A. Drabent, F. de Gasperin, G. Gürkan, G. H. Heald, C. Horellou, B. Nikiel-Wroczynski, R. Paladino, J. Piotrowska, H. J. A. Röttgering, D. J. B. Smith, C. Tasse
Publikováno v:
Astronomy & Astrophysics, 664:A83
Context. Cosmic rays and magnetic fields are key ingredients in galaxy evolution, regulating both stellar feedback and star formation. Their properties can be studied with low-frequency radio continuum observations that are free from thermal contamin
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::adac660be5e6e3be2e4e81f317e0960f
https://ui.adsabs.harvard.edu/abs/2022A&A...664A..83H
https://ui.adsabs.harvard.edu/abs/2022A&A...664A..83H
Akademický článek
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Akademický článek
Tento výsledek nelze pro nepřihlášené uživatele zobrazit.
K zobrazení výsledku je třeba se přihlásit.
K zobrazení výsledku je třeba se přihlásit.