Relevant bibliographies by topics / Intra Cluster Medium

Contents

  1. Journal articles
  2. Dissertations / Theses
  3. Books
  4. Book chapters
  5. Conference papers

Academic literature on the topic 'Intra Cluster Medium'

Author: Grafiati
Published: 11 March 2023
Last updated: 31 July 2025

Create a spot-on reference in APA, MLA, Chicago, Harvard, and other styles

Select a source type:

Consult the lists of relevant articles, books, theses, conference reports, and other scholarly sources on the topic 'Intra Cluster Medium.'

Next to every source in the list of references, there is an 'Add to bibliography' button. Press on it, and we will generate automatically the bibliographic reference to the chosen work in the citation style you need: APA, MLA, Harvard, Chicago, Vancouver, etc.

You can also download the full text of the academic publication as pdf and read online its abstract whenever available in the metadata.

Journal articles on the topic "Intra Cluster Medium"

1

Domainko, Wilfried, Wolfgang Kapferer, Sabine Schindler, Eelco van Kampen, Stefan Kimeswenger, and Maximilian Ruffert. "The Chemical Evolution of the Intra-Cluster Medium." Symposium - International Astronomical Union 217 (2004): 464–65. http://dx.doi.org/10.1017/s0074180900198195.

Full text
Abstract:
We present numerical simulations of the dynamical and chemical evolution of galaxy clusters. from X-ray spectra it is evident that the Intra-Cluster Medium (ICM) is abundant in metals. As heavy elements are only produced in stars the processed material must have been ejected by cluster galaxies into the ICM. Several different mechanisms for interaction between the cluster galaxies and the ICM are possible but their efficiency of metal enrichment of the cluster and their time evolution are still not known. Suggested processes which remove enriched material from the galaxies are ram-pressure str
APA, Harvard, Vancouver, ISO, and other styles
2

Bonafede, Annalisa, Chiara Stuardi, Federica Savini, Franco Vazza, and Marcus Brüggen. "Constraining magnetic fields in galaxy clusters." Proceedings of the International Astronomical Union 14, A30 (2018): 299–302. http://dx.doi.org/10.1017/s1743921319004459.

Full text
Abstract:
AbstractMagnetic fields originate small-scale instabilities in the plasma of the intra-cluster medium, and may have a key role to understand particle acceleration mechanisms. Recent observations at low radio frequencies have revealed that synchrotron emission from galaxy clusters is more various and complicated than previously thought, and new types of radio sources have been observed. In the last decade, big steps forward have been done to constrain the magnetic field properties in clusters thanks to a combined approach of polarisation observations and numerical simulations that aim to reprod
APA, Harvard, Vancouver, ISO, and other styles
3

Schindler, S. "Metal Enrichment in the Intra-Cluster Medium." EAS Publications Series 24 (2007): 121–32. http://dx.doi.org/10.1051/eas:2007019.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Moretti, A., L. Portinari, and C. Chiosi. "Chemical evolution of the intra-cluster medium." Astronomy & Astrophysics 408, no. 2 (2003): 431–53. http://dx.doi.org/10.1051/0004-6361:20031012.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Kotecha, Sachin, Charlotte Welker, Zihan Zhou, et al. "Cosmic filaments delay quenching inside clusters." Monthly Notices of the Royal Astronomical Society 512, no. 1 (2022): 926–44. http://dx.doi.org/10.1093/mnras/stac300.

Full text
Abstract:
ABSTRACT We investigate how large-scale cosmic filaments impact the quenching of galaxies within one virial radius of 324 simulated clusters from The Three Hundred project. We track cosmic filaments with the versatile, observation-friendly program DisPerSE and identify haloes hosting galaxies with VELOCIRaptor. We find that cluster galaxies close to filaments tend to be more star forming, bluer, and contain more cold gas than their counterparts further away from filaments. This effect is recovered at all stellar masses. This is in stark contrast with galaxies residing outside of clusters, wher
APA, Harvard, Vancouver, ISO, and other styles
6

Bignamini, A., P. Tozzi, S. Borgani, S. Ettori, and P. Rosati. "Intra cluster medium properties and AGN distribution in high-zRCS clusters." Astronomy & Astrophysics 489, no. 3 (2008): 967–79. http://dx.doi.org/10.1051/0004-6361:200809437.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Cucchetti, E., N. Clerc, E. Pointecouteau, P. Peille, and F. Pajot. "Towards mapping turbulence in the intra-cluster medium." Astronomy & Astrophysics 629 (September 2019): A144. http://dx.doi.org/10.1051/0004-6361/201935677.

Full text
Abstract:
X-ray observations of the hot gas filling the intra-cluster medium (ICM) provide a wealth of information on the dynamics of clusters of galaxies. The global equilibrium of the ICM is believed to be ensured by non-thermal and thermal pressure support sources, among which gas movements and the dissipation of energy through turbulent motions. Accurate mapping of turbulence using X-ray emission lines is challenging due to the lack of spatially resolved spectroscopy. Only future instruments such as the X-ray Integral Field Unit (X-IFU) on Athena will have the spatial and spectral resolution to quan
APA, Harvard, Vancouver, ISO, and other styles
8

Schindler, S., W. Kapferer, W. Domainko, et al. "Metal enrichment processes in the intra-cluster medium." Astronomy & Astrophysics 435, no. 2 (2005): L25—L28. http://dx.doi.org/10.1051/0004-6361:200500107.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Puchwein, E., and M. Bartelmann. "Three-dimensional reconstruction of the intra-cluster medium." Astronomy & Astrophysics 455, no. 3 (2006): 791–801. http://dx.doi.org/10.1051/0004-6361:20054717.

Full text
APA, Harvard, Vancouver, ISO, and other styles
10

Clerc, Nicolas, Edoardo Cucchetti, Etienne Pointecouteau, and Philippe Peille. "Towards mapping turbulence in the intra-cluster medium." Astronomy & Astrophysics 629 (September 2019): A143. http://dx.doi.org/10.1051/0004-6361/201935676.

Full text
Abstract:
Context. X-ray observations of galaxy clusters provide insights into the nature of gaseous turbulent motions, their physical scales, and the fundamental processes to which they are related. Spatially-resolved, high-resolution spectral measurements of X-ray emission lines provide diagnostics on the nature of turbulent motions in emitting atmospheres. Since they are acting on scales comparable to the size of the objects, the uncertainty on these physical parameters is limited by the number of observational measurements, through sample variance. Aims. We propose a different and complementary appr
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "Intra Cluster Medium"

1

Ghirardini, Vittorio <1990&gt. "Mapping of the intra-cluster medium out to the virial radius." Doctoral thesis, Alma Mater Studiorum - Università di Bologna, 2019. http://amsdottorato.unibo.it/8775/1/thesis.pdf.

Full text
Abstract:
In this thesis, I study the thermodynamic properties of the intracluster medium out to the virial radius, making use of a unique combination of dedicated XMM-Newton exposures and Planck maps, thus exploiting the capabilities of multi-wavelength observations, to constrain at an unprecedented level the thermodynamic properties in a complete sample of galaxy clusters. I will explore in detail their self-similar properties, their radial dependence, and their implication. This work provides an important legacy value for any future studies of galaxy cluster until the next generation of X-ray teles
APA, Harvard, Vancouver, ISO, and other styles
2

LECCARDI, ALBERTO. "Thermodynamic and chemical properties of the intra-cluster medium in the outer regions of galaxy clusters." Doctoral thesis, Università degli Studi di Milano, 2009. http://hdl.handle.net/2434/72734.

Full text
Abstract:
Clusters of galaxies are the most massive gravitationally bound systems in the universe. They are permeated by a hot, X-ray emitting, intra-cluster medium (ICM), which represents the dominant baryonic component. The key ICM observable quantities are its density, temperature, and chemical composition (in particular, the so-called metallicity). Measuring the gas density is relatively simple, whereas measuring the temperature and the metallicity of the ICM requires accumulating a spectrum and fitting it with a plasma model. The aim of my thesis is the characterization of the radial propertie
APA, Harvard, Vancouver, ISO, and other styles
3

Fabjan, Dunja. "The effect of star formation and feedback on the X-ray properties of simulated galaxy clusters." Doctoral thesis, Università degli studi di Trieste, 2010. http://hdl.handle.net/10077/3434.

Full text
Abstract:
2008/2009<br>The aim of this Thesis was to study the X--ray properties of the IntraCluster Medium (ICM) in a cosmological context resorting to high resolution hydrodynamical simulations. The thermodynamical and chemical properties of the ICM were inspected and studied within a set of galaxy clusters that were simulated with the TREE-SPH Gadget2 code (Springel 2005). This code included a detailed model of chemical evolution (Tornatore et al. 2007) as well as prescriptions for different physical processes: star formation, galactic winds and AGN feedback. We use this large set of simulated gala
APA, Harvard, Vancouver, ISO, and other styles
4

Ruppin, Florian. "Cosmologie via les observations d'amas de galaxies par effet Sunyaev-Zel'dovich avec NIKA2." Thesis, Université Grenoble Alpes (ComUE), 2018. http://www.theses.fr/2018GREAY029/document.

Full text
Abstract:
La distribution de masse dans l'Univers telle que tracée par les amas de galaxies constitue une sonde cosmologique puissante. La caractérisation des processus associés à l'origine et à la croissance des grandes structures permet de contraindre des paramètres cosmologiques via l'étude de la distribution des amas en fonction de leur masse et de leur redshift. Cependant, il existe un désaccord statistiquement significatif observé entre les contraintes cosmologiques établies par l'étude des anisotropies primaires du fond diffus cosmologique et celles issues de l'analyse de la distribution des amas
APA, Harvard, Vancouver, ISO, and other styles
5

Balestra, Italo [Verfasser]. "Elemental abundances in the intra-cluster medium and in active galactic nuclei / Italo Balestra." 2007. http://d-nb.info/987922483/34.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Rhea, Carter. "Nouvelles observations et techniques d'apprentissage automatique appliquées aux galaxies et aux amas de galaxies." Thesis, 2020. http://hdl.handle.net/1866/24376.

Full text
Abstract:
Les amas de galaxies sont l'une des plus grandes structures dans l'univers et jouent le rôle d'hôte de plusieurs phénomènes complexes. Bien qu'il existe beaucoup d'études portant sur leur formation et leur évolution, l'avènement récent de l'apprentissage automatique en astronomie nous permet d'investiguer des questions qui, jusqu'à maintenant, demeuraient sans réponse. Même si ce mémoire se concentre sur l'application de techniques d'apprentissage automatique aux observations en rayons X des amas de galaxies, nous explorons l'usage de ces techniques à son homologue à une échelle réduite : les
APA, Harvard, Vancouver, ISO, and other styles
7

Latulippe, Myriam. "Influence du trou noir supermassif central dans l’amas de galaxies MACS J1447.4+0827." Thèse, 2017. http://hdl.handle.net/1866/20312.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Gendron-Marsolais, Marie-Lou. "Observations multi-longueur d’onde d’amas et de groupes de galaxies proches." Thèse, 2018. http://hdl.handle.net/1866/21757.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Richard-Laferrière, Annabelle. "L'impact des trous noirs les plus massifs de l’Univers sur le coeur des amas de galaxies." Thèse, 2019. http://hdl.handle.net/1866/22724.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Books on the topic "Intra Cluster Medium"

1

The environmental impact of intra-cluster medium on the interstellar medium in early type galaxies: Semiannual reports, 1 August 1993-31 January 1994 ... 1 August 1994-31 January 1995, annual report, 1 August 1995-31 July 1996. Smithsonian Institution, Astrophysical Observatory, 1996.

Find full text
APA, Harvard, Vancouver, ISO, and other styles

Book chapters on the topic "Intra Cluster Medium"

1

Cora, Sofía A., and Simon D. M. White. "Chemical Enrichment of the Intra-Cluster Medium." In The Evolution of Galaxies. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-3315-1_23.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Elbaz, D., and L. Vigroux. "Timescales for Galaxy Formation and Intra-Cluster Medium Enrichment." In New Light on Galaxy Evolution. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0229-9_82.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Iapichino, Luigi, Jens C. Niemeyer, Surajit Paul, and Wolfram Schmidt. "Turbulence Modeling and the Physics of the Intra-Cluster Medium." In High Performance Computing in Science and Engineering, Garching/Munich 2009. Springer Berlin Heidelberg, 2010. http://dx.doi.org/10.1007/978-3-642-13872-0_32.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Ulmer, M. P., R. G. Cruddace, E. Fenimore, W. A. Snyder, and G. Fritz. "Elemental Abundances and Temperature Distributions in the Intra-Cluster Medium of the Perseus Cluster." In Observational Cosmology. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3853-3_51.

Full text
APA, Harvard, Vancouver, ISO, and other styles

Conference papers on the topic "Intra Cluster Medium"

1

Molendi, Silvano. "The Intra-Cluster Medium." In PLASMAS IN THE LABORATORY AND IN THE UNIVERSE: New Insights and New Challenges. AIP, 2004. http://dx.doi.org/10.1063/1.1718479.

Full text
APA, Harvard, Vancouver, ISO, and other styles
2

Domainko, Wilfried, W. Kapferer, M. Gitti, et al. "Metal enrichment of the Intra-Cluster Medium: Ram-Pressure Stripping and Feedback from Intra-Cluster Supernovae." In Baryons in Dark Matter Halos. Sissa Medialab, 2004. http://dx.doi.org/10.22323/1.014.0074.

Full text
APA, Harvard, Vancouver, ISO, and other styles
3

Molendi, Silvano, A. Comastri, L. Angelini, and M. Cappi. "The Intra-cluster medium: recent results and future prospects." In X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3475229.

Full text
APA, Harvard, Vancouver, ISO, and other styles
4

Iapichino, L., A. Maier, W. Schmidt, J. C. Niemeyer, Jean-Michel Alimi, and André Fuözfa. "Turbulence modeling and the physics of the intra-cluster medium." In INVISIBLE UNIVERSE: Proceedings of the Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3462735.

Full text
APA, Harvard, Vancouver, ISO, and other styles
5

Basu, K., M. W. Sommer, Y. Y. Zhang, A. Comastri, L. Angelini, and M. Cappi. "Joint X-ray∕Sunyaev-Zel’dovich Analysis of the Intra-Cluster Medium." In X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3475230.

Full text
APA, Harvard, Vancouver, ISO, and other styles
6

Sato, Kosuke, Kazuyo Tokoi, Kyoko Matsushita, et al. "Supernovae contributions to metals in intra-cluster medium observed with Suzaku." In ORIGIN OF MATTER AND EVOLUTION OF GALAXIES: The 10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System. AIP, 2008. http://dx.doi.org/10.1063/1.2943599.

Full text
APA, Harvard, Vancouver, ISO, and other styles
7

Schindler, Sabine. "Interaction of galaxies with the intra-cluster medium and ICM metal enrichment." In Baryons in Dark Matter Halos. Sissa Medialab, 2004. http://dx.doi.org/10.22323/1.014.0023.

Full text
APA, Harvard, Vancouver, ISO, and other styles
8

Pančišin, M., C. Kaiser, G. Pavlovski, et al. "Enrichment of the Intra-Cluster Medium Due to AGN Outflows Induced by Late-Type Galaxies." In THE MONSTER’S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS. AIP, 2009. http://dx.doi.org/10.1063/1.3293015.

Full text
APA, Harvard, Vancouver, ISO, and other styles
9

Liu, Wing Kam, and Ashfaq Adnan. "Multiscale Modeling and Simulation for Nanodiamond-Based Therapeutic Delivery." In ASME 2010 First Global Congress on NanoEngineering for Medicine and Biology. ASMEDC, 2010. http://dx.doi.org/10.1115/nemb2010-13273.

Full text
Abstract:
It has been demonstrated from recent research that nanodiamond(ND)-enabled drug delivery as cancer therapeutics represents an important component of optimized device functionality. The goal of the current research is to develop a multiscale modeling technique to understand the fundamental mechanism of a ND-based cancer therapeutic drug delivery system. The major components of the proposed device include nanodiamonds (ND), parylene buffer layer and doxorubicin (DOX) drugs, where DOX loaded self-assembled nanodiamonds are packed inside parylene capsule. The efficient functioning of the device is
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'Intra Cluster Medium' for particular source types:
Journal articles
We offer discounts on all premium plans for authors whose works are included in thematic literature selections. Contact us to get a unique promo code!

To the bibliography