Zobrazeno 1 - 10
of 1 319
pro vyhledávání: '"P. van Weeren"'
Autor:
Oei, Martijn S. S. L., Hardcastle, Martin J., Timmerman, Roland, Gast, Aivin R. D. J. G. I. B., Botteon, Andrea, Rodriguez, Antonio C., Stern, Daniel, Rivera, Gabriela Calistro, van Weeren, Reinout J., Röttgering, Huub J. A., Intema, Huib T., de Gasperin, Francesco, Djorgovski, S. G.
Publikováno v:
Nature, 2024, Volume 633, Issue 8030, Pages 537--541
Jets launched by supermassive black holes transport relativistic leptons, magnetic fields, and atomic nuclei from the centres of galaxies to their outskirts and beyond. These outflows embody the most energetic pathway by which galaxies respond to the
Externí odkaz:
http://arxiv.org/abs/2411.08630
Autor:
Morabito, Leah K., Kondapally, R., Best, P. N., Yue, B. -H., de Jong, J. M. G. H. J., Sweijen, F., Bondi, Marco, Schwarz, Dominik J., Smith, D. J. B., van Weeren, R. J., Röttgering, H. J. A., Shimwell, T. W., Prandoni, Isabella
Both star formation (SF) and Active Galactic Nuclei (AGN) play an important role in galaxy evolution. Statistically quantifying their relative importance can be done using radio luminosity functions. Until now these relied on galaxy classifications,
Externí odkaz:
http://arxiv.org/abs/2411.05069
Autor:
Lepore, M., Pinto, C., Tozzi, P., Gaspari, M., Gastaldello, F., Liu, A., Rosati, P., van Weeren, R., Cresci, G., Iani, E., Rodighiero, G.
We present a detailed analysis of the thermal X-ray emission from the intracluster medium (ICM) in the cool-core galaxy cluster Abell 2667 ($z=0.23$). Our goal is to detect low-temperature ($<2$ keV) X-ray emitting gas, potentially associated to a co
Externí odkaz:
http://arxiv.org/abs/2410.16831
Autor:
van Weeren, R. J., Timmerman, R., Vaidya, V., Gendron-Marsolais, M. -L., Botteon, A., Roberts, I. D., Hlavacek-Larrondo, J., Bonafede, A., Brüggen, M., Brunetti, G., Cassano, R., Cuciti, V., Edge, A. C., Gastaldello, F., Groeneveld, C., Shimwell, T. W.
The Perseus cluster is the brightest X-ray cluster in the sky and is known as a cool-core galaxy cluster. Being a very nearby cluster, it has been extensively studied. This has provided a comprehensive view of the physical processes that operate in t
Externí odkaz:
http://arxiv.org/abs/2410.02863
Autor:
Pignataro, G. V., Bonafede, A., Bernardi, G., Balboni, M., Vazza, F., van Weeren, R. J., Ubertosi, F., Cassano, R., Brunetti, G., Botteon, A., Venturi, T., Akamatsu, H., Drabent, A., Hoeft, M.
The clusters Abell 2061 and Abell 2067 in the Corona Borealis supercluster have been studied at different radio frequencies and are both known to host diffuse radio emission. The aim of this work is to investigate the radio emission in between them,
Externí odkaz:
http://arxiv.org/abs/2409.15412
Autor:
Bruno, L., Venturi, T., Dallacasa, D., Brienza, M., Ignesti, A., Brunetti, G., Riseley, C. J., Rossetti, M., Gastaldello, F., Botteon, A., Rudnick, L., van Weeren, R. J., Shulevski, A., Lal, D. V.
Publikováno v:
A&A 690, A329 (2024)
Context. Tailed radio galaxies are shaped by ram pressure owing to the high-velocity motion of their host through the intracluster medium (ICM). Recent works have reported on the increasing complexity of the phenomenology of tailed galaxies, with dep
Externí odkaz:
http://arxiv.org/abs/2409.03453
Autor:
De Rubeis, E., Stuardi, C., Bonafede, A., Vazza, F., van Weeren, R. J., de Gasperin, F., Brüggen, M.
Publikováno v:
A&A 691, A23 (2024)
In this paper, we investigate the polarization properties of the double radio relics in PSZ2 G096.88+24.18 using the rotation measure synthesis, and try to constrain the characteristics of the magnetic field that reproduce the observed beam depolariz
Externí odkaz:
http://arxiv.org/abs/2408.08603
Autor:
Osinga, Erik, van Weeren, Reinout J., Rudnick, Lawrence, Andrade-Santos, Felipe, Bonafede, Annalisa, Clarke, Tracy, Duncan, Kenda, Giacintucci, Simona, Röttgering, Huub J. A.
Magnetic fields remain an enigmatic part of the content of galaxy clusters. Faraday rotation and depolarisation of extragalactic radio sources are useful probes, but the limited availability of polarised radio sources necessitates stacking clusters t
Externí odkaz:
http://arxiv.org/abs/2408.07178
Autor:
de Jong, J. M. G. H. J., van Weeren, R. J., Sweijen, F., Oonk, J. B. R., Shimwell, T. W., Offringa, A. R., Morabito, L. K., Röttgering, H. J. A., Kondapally, R., Escott, E. L., Best, P. N., Bondi, M., Ye, H., Petley, J. W.
We present the deepest wide-field 115-166 MHz image at sub-arcsecond resolution spanning an area of 2.5 by 2.5 degrees centred at the ELAIS-N1 deep field. To achieve this, we improved the calibration for the International LOFAR Telescope. This enhanc
Externí odkaz:
http://arxiv.org/abs/2407.13247
Autor:
Finner, Kyle, Jee, M. James, Cho, Hyejeon, Hyeonghan, Kim, Lee, Wonki, van Weeren, Reinout J., Wittman, David, Yoon, Mijin
We present a multiwavelength analysis of 29 merging galaxy clusters that exhibit radio relics. For each merging system, we perform a weak-lensing analysis on Subaru optical imaging. We generate high-resolution mass maps of the dark matter distributio
Externí odkaz:
http://arxiv.org/abs/2407.02557