Zobrazeno 1 - 10
of 1 485
pro vyhledávání: '"Grandi, S"'
Autor:
Bartalucci, I., Rossetti, M., Boschin, W., Girardi, M., Nonino, M., Baraldi, E., Balboni, M., Coe, D., De Grandi, S., Gastaldello, F., Ghizzardi, S., Giacintucci, S., Grillo, C., Harvey, D., Lovisari, L., Molendi, S., Resseguier, T., Riva, G., Venturi, T., Zitrin, A.
We present a detailed study of the gas and galaxy properties of the cluster PSZ2 G282.28+49.94 detected in the Planck all-sky survey. The intracluster medium (ICM) of this object at z=0.56 exhibits a cometary-like shape. Combining Chandra and TNG obs
Externí odkaz:
http://arxiv.org/abs/2409.07290
Autor:
Molendi, S., Ghizzardi, S., De Grandi, S., Balboni, M., Bartalucci, I., Eckert, D., Gastaldello, F., Lovisari, L., Riva, G., Rossetti, M.
Aims. The goal of this work is to devise a description of the enrichment process in large-scale structure that explains the available observations and makes predictions for future measurements. Methods. We took a spartan approach to this study, emplo
Externí odkaz:
http://arxiv.org/abs/2403.03987
Autor:
Balboni, M., Gastaldello, F., Bonafede, A., Botteon, A., Bartalucci, I., Bourdin, H., Brunetti, G., Cassano, R., De Grandi, S., De Luca, F., Ettori, S., Ghizzardi, S., Gitti, M., Iqbal, A., Johnston-Hollitt, M., Lovisari, L., Mazzotta, P., Molendi, S., Pointecouteau, E., Pratt, G. W., Riva, G., Rossetti, M., Rottgering, H., Sereno, M., van Weeren, R. J., Venturi, T., Veronesi, I.
The connection between the thermal and non-thermal properties in galaxy clusters hosting radio halos seems fairly well established. However, a comprehensive analysis of such a connection has been made only for integrated quantities (e.g. $L_X - P_{ra
Externí odkaz:
http://arxiv.org/abs/2402.18654
Autor:
Rossetti, M., Eckert, D., Gastaldello, F., Rasia, E., Pratt, G. W., Ettori, S., Molendi, S., Arnaud, M., Balboni, M., Bartalucci, I., Batalha, R. M., Borgani, S., Bourdin, H., De Grandi, S., De Luca, F., De Petris, M., Forman, W., Gaspari, M., Ghizzardi, S., Iqbal, A., Kay, S., Lovisari, L., Maughan, B. J., Mazzotta, P., Pointecouteau, E., Riva, G., Sayers, J., Sereno, M.
Publikováno v:
A&A 686, A68 (2024)
The "Cluster HEritage project with \xmm: Mass Assembly and Thermodynamics at the Endpoint of structure formation" (CHEX-MATE) is a multi-year Heritage program, to obtain homogeneous XMM-Newton observations of a representative sample of 118 galaxy clu
Externí odkaz:
http://arxiv.org/abs/2402.18653
Autor:
Lovisari, L., Ettori, S., Rasia, E., Gaspari, M., Bourdin, H., Campitiello, M. G., Rossetti, M., Bartalucci, I., De Grandi, S., De Luca, F., De Petris, M., Eckert, D., Forman, W., Gastaldello, F., Ghizzardi, S., Jones, C., Kay, S., Kim, J., Maughan, B. J., Mazzotta, P., Pointecouteau, E., Pratt, G. W., Sayers, J., Sereno, M., Simonte, M., Tozzi, P.
Publikováno v:
A&A 682, A45 (2024)
We study the perturbations in the temperature (and density) distribution for 28 clusters selected from the CHEX-MATE sample to evaluate and characterize the level of inhomogeneities and the related dynamical state of the ICM. We use these spatially r
Externí odkaz:
http://arxiv.org/abs/2311.02176
Autor:
Bruno, L., Botteon, A., Shimwell, T., Cuciti, V., de Gasperin, F., Brunetti, G., Dallacasa, D., Gastaldello, F., Rossetti, M., van Weeren, R. J., Venturi, T., Russo, S. A., Taffoni, G., Cassano, R., Biava, N., Lusetti, G., Bonafede, A., Ghizzardi, S., De Grandi, S.
Publikováno v:
A&A 678, A133 (2023)
Turbulence introduced into the intra-cluster medium (ICM) through cluster merger events transfers energy to non-thermal components, and can trigger the formation of diffuse synchrotron radio sources. Typical diffuse sources in the forms of giant radi
Externí odkaz:
http://arxiv.org/abs/2308.07603
Autor:
Bartalucci, I., Molendi, S., Rasia, E., Pratt, G. W., Arnaud, M., Rossetti, M., Gastaldello, F., Eckert, D., Balboni, M., Borgani, S., Bourdin, H., Campitiello, M. G., De Grandi, S., De Petris, M., Duffy, R. T., Ettori, S., Ferragamo, A., Gaspari, M., Gavazzi, R., Ghizzardi, S., Iqbal, A., Kay, S. T., Lovisari, L., Mazzotta, P., Maughan, B. J., Pointecouteau, E., Riva, G., Sereno, M.
Publikováno v:
A&A 674, A179 (2023)
We investigate the statistical properties and the origin of the scatter within the spatially resolved surface brightness profiles of the CHEX-MATE sample, formed by 118 galaxy clusters selected via the SZ effect. These objects have been drawn from th
Externí odkaz:
http://arxiv.org/abs/2305.03082
Autor:
Boschin, W., Girardi, M., De Grandi, S., Riva, G., Feretti, L., Giovannini, G., Govoni, F., Vacca, V.
Publikováno v:
A&A 672, A199 (2023)
Context. Abell 1213, a low-richness galaxy system, is known to host an anomalous radio halo detected in data of the VLA. It is an outlier with regard to the relation between the radio halo power and the X-ray luminosity of the parent clusters. Aims.
Externí odkaz:
http://arxiv.org/abs/2303.02528
Autor:
Molendi, S., De Grandi, S., Rossetti, M., Bartalucci, I., Gastaldello, F., Ghizzardi, S., Gaspari, M.
Publikováno v:
A&A 670, A104 (2023)
In this work we address the issue of whether the division of clusters in cool cores (CCs) and non-cool cores (NCCs) is due to a primordial difference or to how clusters evolve across cosmic time. Our first goal is to establish if spectra from the cen
Externí odkaz:
http://arxiv.org/abs/2210.14148
Autor:
Riva, G., Ghizzardi, S., Molendi, S., Bartalucci, I., De Grandi, S., Gastaldello, F., Grillo, C., Rossetti, M.
Publikováno v:
A&A 665, A81 (2022)
In intermediate-temperature (T = 2.5 - 4.5 keV) galaxy clusters, abundance measurements are almost-equally driven by Fe K and L transitions, at $\sim$ 6.7 keV and 0.9 - 1.3 keV, respectively. While K-shell-derived measurements are considered reliable
Externí odkaz:
http://arxiv.org/abs/2206.14827