Zobrazeno 1 - 4
of 4
pro vyhledávání: '"Timothy Shimwell"'
Autor:
Kohei Kurahara, Takuya Akahori, Ruta Kale, Hiroki Akamatsu, Yutaka Fujita, Liyi Gu, Huib Intema, Kazuhiro Nakazawa, Nobuhiro Okabe, Yuki Omiya, Viral Parekh, Timothy Shimwell, Motokazu Takizawa, Reinout J Van Weeren
Publikováno v:
Publications of Astronomical Society of Japan, 75(Supplement 1), S138-S153
We report on results of our upgraded Giant Metrewave Radio Telescope (uGMRT) observations for an early-stage merging galaxy cluster, CIZA J1358.9-4750 (CIZA1359), in Band-3 (300--500 MHz). We achieved the image dynamic range of $\sim 38,000$ using th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::140c49b6abdf3e5528205f494ad660ea
http://hdl.handle.net/1887/3514246
http://hdl.handle.net/1887/3514246
Autor:
Alessandro Ignesti, Benedetta Vulcani, Bianca M. Poggianti, Rosita Paladino, Timothy Shimwell, Julia Healy, Myriam Gitti, Cecilia Bacchini, Alessia Moretti, Mario Radovich, Reinout J. van Weeren, Ian D. Roberts, Andrea Botteon, Ancla Müller, Sean McGee, Jacopo Fritz, Neven Tomičić, Ariel Werle, Matilde Mingozzi, Marco Gullieuszik, Marc Verheijen
Publikováno v:
Astrophysical Journal, 924(2):64. IOP PUBLISHING LTD
The Astrophysical Journal, 924(2):64
The Astrophysical Journal, 924(2):64
Ram pressure stripping is a crucial evolutionary driver for cluster galaxies. It is thought to be able to accelerate the evolution of their star formation, trigger the activity of their central active galactic nucleus (AGN) and the interplay between
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::517206832840facc5c8abdbc4986a0b3
https://research.rug.nl/en/publications/d9efa7e4-7907-4eeb-9462-32cd67131707
https://research.rug.nl/en/publications/d9efa7e4-7907-4eeb-9462-32cd67131707
Autor:
Marcin Hajduk, Paolo Leto, Harish Vedantham, Corrado Trigilio, Marijke Haverkorn, Timothy Shimwell, Joseph R. Callingham, Glenn J. White
Publikováno v:
Astronomy & Astrophysics, 665, 1-6
Astronomy & Astrophysics, 665:A152
Astronomy & Astrophysics, 665, pp. 1-6
Astronomy & Astrophysics, 665:A152
Astronomy & Astrophysics, 665, pp. 1-6
Context. Chemically peculiar stars are upper main sequence stars that show anomalies in their optical spectra. These anomalies suggest peculiar chemical abundances of certain elements. Some chemically peculiar stars possess strong magnetic fields. El
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::a80860f75b11ae2e5be57da22f41c937
http://hdl.handle.net/2066/282478
http://hdl.handle.net/2066/282478
Autor:
Alessandro Ignesti, Benedetta Vulcani, Bianca M. Poggianti, Alessia Moretti, Timothy Shimwell, Andrea Botteon, Reinout J. van Weeren, Ian D. Roberts, Jacopo Fritz, Neven Tomičić, Giorgia Peluso, Rosita Paladino, Myriam Gitti, Ancla Müller, Sean McGee, Marco Gullieuszik
Publikováno v:
The Astrophysical Journal, 937(2):58
Jellyfish galaxies, characterized by long filaments of stripped interstellar medium extending from their disks, are the prime laboratories to study the outcomes of ram pressure stripping. At radio wavelengths, they often show unilateral emission exte
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::c2b18546c0174bd20221229e6b254062
https://ui.adsabs.harvard.edu/abs/2022ApJ...937...58I
https://ui.adsabs.harvard.edu/abs/2022ApJ...937...58I