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Relevant bibliographies by topics / Galaxy clusters/dynamics study

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Academic literature on the topic 'Galaxy clusters/dynamics study'

Author: Grafiati

Published: 4 June 2021

Last updated: 2 February 2022

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Journal articles on the topic "Galaxy clusters/dynamics study"

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Benavides, José A., Laura V. Sales, and Mario G. Abadi. "Accretion of galaxy groups into galaxy clusters." Monthly Notices of the Royal Astronomical Society 498, no. 3 (2020): 3852–62. http://dx.doi.org/10.1093/mnras/staa2636.

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ABSTRACT We study the role of group infall in the assembly and dynamics of galaxy clusters in ΛCDM. We select 10 clusters with virial mass M200 ∼ 1014 $\rm M_\odot$ from the cosmological hydrodynamical simulation Illustris and follow their galaxies with stellar mass M⋆ ≥ 1.5 × 108 $\rm M_\odot$. A median of ${\sim}38{{\ \rm per\ cent}}$ of surviving galaxies at z = 0 is accreted as part of groups and did not infall directly from the field, albeit with significant cluster-to-cluster scatter. The evolution of these galaxy associations is quick, with observational signatures of their common origi

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Valenti, E., L. Origlia, and R. M. Rich. "Globular clusters in the near–infrared." Proceedings of the International Astronomical Union 5, H15 (2009): 555–56. http://dx.doi.org/10.1017/s1743921310010719.

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The study of Globular Cluster (GC) stellar populations (SPs) addresses fundamental astrophysical questions ranging from stellar structure, evolution and dynamics, to Galaxy formation. Indeed, they represent: i) fossils from the remote and violent epoch of Galaxy formation, ii) test particles for studying Galaxy dynamics and stellar dynamical model, and iii) fiducial templates for studying integrated light from distant stellar systems. In particular, high resolution spectroscopy of GC SPs provides abundance patterns which are crucial for understanding the formation and chemical enrichment time–

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Savini, F., A. Bonafede, M. Brüggen, et al. "A LOFAR study of non-merging massive galaxy clusters." Astronomy & Astrophysics 622 (February 2019): A24. http://dx.doi.org/10.1051/0004-6361/201833882.

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Centrally located diffuse radio emission has been observed in both merging and non-merging galaxy clusters. Depending on their morphology and size, we distinguish between giant radio haloes, which occur predominantly in merging clusters, and mini haloes, which are found in non-merging, cool-core clusters. In recent years, cluster-scale radio emission has also been observed in clusters with no sign of major mergers, showing that our knowledge of the mechanisms that lead to particle acceleration in the intra-cluster medium (ICM) is still incomplete. Low-frequency sensitive observations are requi

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John, Reju Sam, Surajit Paul, Luigi Iapichino, Karl Mannheim, and Harish Kumar. "Manufacturing cosmic rays in the evolving dynamical states of galaxy clusters." Monthly Notices of the Royal Astronomical Society 488, no. 1 (2019): 1301–19. http://dx.doi.org/10.1093/mnras/stz1785.

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ABSTRACT Galaxy clusters are known to be reservoirs of cosmic rays (CRs), as inferred from theoretical calculations or detection of CR-derived observables. CR acceleration in clusters is mostly attributed to the dynamical activity that produces shocks. Shocks in clusters emerge out of merger or accretion, but which one is more effective in producing CRs? at which dynamical phase? and why? To this aim, we study the production or injection of CRs through shocks and its evolution in the galaxy clusters using cosmological simulations with the enzo code. Particle acceleration model considered here

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Roberts, Ian D., and Laura C. Parker. "‘Observing’ unrelaxed clusters in dark matter simulations." Monthly Notices of the Royal Astronomical Society 490, no. 1 (2019): 773–83. http://dx.doi.org/10.1093/mnras/stz2666.

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ABSTRACT We present a detailed study of relaxed and unrelaxed galaxy clusters in a large dark matter only simulation. Recent work has demonstrated clear differences between the galaxy populations in clusters that have Gaussian velocity distributions (relaxed) compared to those that do not (unrelaxed). To directly compare with observations, we identify unrelaxed clusters in the simulations using one-dimensional velocity distributions. We show that non-Gaussian clusters have had recent major mergers and enhanced rates of galaxy infall relative to systems with Gaussian velocity profiles. Furtherm

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Cuciti, V., R. Cassano, G. Brunetti, et al. "Radio halos in a mass-selected sample of 75 galaxy clusters." Astronomy & Astrophysics 647 (March 2021): A51. http://dx.doi.org/10.1051/0004-6361/202039208.

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Context. Many galaxy clusters host megaparsec-scale diffuse radio sources called radio halos. Their origin is tightly connected to the processes that lead to the formation of clusters themselves. In order to reveal this connection, statistical studies of the radio properties of clusters combined with their thermal properties are necessary. For this purpose, we selected a sample of galaxy clusters with M500 ≥ 6 × 1014 M⊙ and z = 0.08 − 0.33 from the Planck Sunyaev–Zel’dovich catalogue. In Paper I, we presented the radio and X-ray data analysis that we carried out on the clusters of this sample.

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Botteon, A., R. Cassano, D. Eckert, et al. "Particle acceleration in a nearby galaxy cluster pair: the role of cluster dynamics." Astronomy & Astrophysics 630 (September 24, 2019): A77. http://dx.doi.org/10.1051/0004-6361/201936022.

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Context. Diffuse radio emission associated with the intracluster medium (ICM) is observed in a number of merging galaxy clusters. It is currently believed that a fraction of the kinetic energy in mergers is channeled into nonthermal components, such as turbulence, cosmic rays, and magnetic fields, which may lead to the formation of giant synchrotron sources in the ICM. Aims. Studying merging galaxy clusters in different evolutionary phases is fundamental for understanding the origin of radio emission in the ICM. Methods. We observed the nearby galaxy cluster pair RXC J1825.3+3026 (z ∼ 0.065) a

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Einasto, Maret, Boris Deshev, Heidi Lietzen, et al. "Infalling groups and galaxy transformations in the cluster A2142." Astronomy & Astrophysics 610 (February 2018): A82. http://dx.doi.org/10.1051/0004-6361/201731600.

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Context. Superclusters of galaxies provide dynamical environments for the study of the formation and evolution of structures in the cosmic web from galaxies, to the richest galaxy clusters, and superclusters themselves. Aims. We study galaxy populations and search for possible merging substructures in the rich galaxy cluster A2142 in the collapsing core of the supercluster SCl A2142, which may give rise to radio and X-ray structures in the cluster, and affect galaxy properties of this cluster. Methods. We used normal mixture modelling to select substructure of the cluster A2142. We compared al

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Stasyszyn, F. A., and M. de los Rios. "Faraday rotation measure dependence on galaxy cluster dynamics." Monthly Notices of the Royal Astronomical Society 487, no. 4 (2019): 4768–74. http://dx.doi.org/10.1093/mnras/stz1450.

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ABSTRACT We study the magnetic fields in galaxy clusters through Faraday rotation measurements crossing systems in different dynamical states. We confirm that magnetic fields are present in those systems and analyse the difference between relaxed and unrelaxed samples with respect to the dispersion between their inherent Faraday rotation measurements (RM). We found an increase of this RM dispersion and a higher RM overlapping frequency for unrelaxed clusters. This fact suggests that a large-scale physical process is involved in the nature of unrelaxed systems and possible depolarization effect

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Peña, J. H., and R. Peniche. "Photometry of early type stars in open clusters (NGC 1444, NGC 1662, NGC 2129, NGC 2169 and NGC 7209)." Symposium - International Astronomical Union 162 (1994): 303–4. http://dx.doi.org/10.1017/s0074180900215143.

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This is part of a series which has the purpose of examining the nature of the stars belonging to open clusters. The aim of this series is, among others things, to study short period pulsating stars, mainly of the Delta Scuti type, by first establishing the membership of each star to the cluster, to determine the abundance of the Be and Ap phenomena and blue stragglers in open clusters for clusters of different ages and metalicities and, eventually, to study the chemical enrichment of the galaxy when age, dynamics and metalicity are known for a fair number of clusters.

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Dissertations / Theses on the topic "Galaxy clusters/dynamics study"

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Millington, S. J. C. "Clusters of galaxies." Thesis, University of Oxford, 1987. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.382461.

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Drake, Nick. "Wakes and dynamics of galaxy clusters." Thesis, University of Southampton, 2000. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.326792.

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Parekh, Viral. "Morphological classification and dynamics of X-ray galaxy clusters." Doctoral thesis, University of Cape Town, 2014. http://hdl.handle.net/11427/9539.

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Braglia, Filiberto Giorgio. "Study of optical properties and galaxy populations of galaxy clusters." Diss., kostenfrei, 2008. http://edoc.ub.uni-muenchen.de/9179/.

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Nastasi, Alessandro. "Multiwavelength Study of high redshift galaxy clusters." Diss., lmu, 2012. http://nbn-resolving.de/urn:nbn:de:bvb:19-152323.

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Hodson, Alistair. "A non-Newtonian perspective of gravity : testing modified gravity theories in galaxies and galaxy clusters." Thesis, University of St Andrews, 2017. http://hdl.handle.net/10023/12016.

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This thesis attempts to test several frameworks of non-Newtonian gravity in the context of galaxies and galaxy clusters. The theory most extensively discussed was that of Modiﬁed Newtonian Dynamics (MOND) with Galileon gravity, Emergent Gravity (EG) and Modiﬁed Gravity (MOG) mentioned to a lesser extent. Speciﬁcally, the main focus of this thesis was to determine whether MOND and MOND-like theories were compatible with galaxy cluster data, without the need to include cold dark matter. To do this, the paradigms of Extended MOND (EMOND), Generalised MOND (GMOND) and superﬂuid dark matter were in

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Moran, Sean M. Djorgovski S. G. Ellis Richard S. "Understanding the physical processes driving galaxy evolution in clusters : a case study of two z~0.5 galaxy clusters /." Diss., Pasadena, Calif. : California Institute of Technology, 2008. http://resolver.caltech.edu/CaltechETD:etd-08212007-151300.

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Winkworth, Carolyn Louise. "An Observational Study of High Redshift Galaxy Clusters." Thesis, University of Bristol, 2009. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.520307.

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Renaud, Florent. "Dynamics of the Tidal Fields and Formation of Star Clusters in Galaxy Mergers." Phd thesis, Université de Strasbourg, 2010. http://tel.archives-ouvertes.fr/tel-00508301.

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Dans les galaxies en interaction, de colossales forces de marée perturbent la morphologie des progéniteurs pour engendrer les longs bras d'étoiles, gaz et poussières que l'on observe parfois. En plus de leur effet destructeur, les forces de marée peuvent, dans certain cas, se placer dans une configuration protectrice appelée mode compressif. De tels modes protègent alors la matière en leur sein, en augmentant son énergie de liaison. Cette thèse se concentre sur l'étude de ce régime peu connu en quantifiant ses propriétés grâce à des outils numériques et analytiques appliqués à un spectaculaire

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Hall, Emily Anne. "Clusters and cosmic onions : a description of galaxy dynamics in the quasi-linear regime." Thesis, University College London (University of London), 2018. http://discovery.ucl.ac.uk/10057210/.

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This thesis investigates the dynamics of galaxies around clusters in the quasi-linear regime, with the ultimate aim of providing cluster mass constraints which can be combined with weak lensing measurements in order to perform tests of General Relativity. Dark matter simulations are populated with galaxies using a halo occupation distribution, and used to develop and test models which describe di↵erent aspects of galaxy dynamics around clusters. A heuristic analytical model is presented describing the infall profile of galaxies onto a cluster of given mass, which is shown to fit the simulation

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Books on the topic "Galaxy clusters/dynamics study"

1

David, Merritt. Galaxy Dynamics: A Rutgers Symposium. Astronomical Society of the Pacific, 1999.

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Hartog, Roland Henrik den. The dynamics of rich galaxy clusters: Proefschrift. Sterrewacht, 1995.

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Blindert, Kris. Internal dynamics of galaxy clusters in the Red-Sequence Cluster Survey. 2006.

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1949-, Lagnevik Magnus, ed. The dynamics of innovation clusters: A study of the food industry. Edward Elgar Pub., 2003.

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Lagnevik, Magnus, Ingegerd Sjoholm, Anders Lareke, and Jacob Ostberg. The Dynamics of Innovation Clusters: A Study of the Food Industry (New Horizons in the Economics of Innovation). Edward Elgar Publishing, 2003.

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6

Danilov, V. M. Non-stationarity of Open Star Clusters. Ural University Press, 2021. http://dx.doi.org/10.15826/b978-5-7996-3173-4.

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The monograph poses issues related to the study of the non-stationarity of open star clusters (OSCs), starting with an analysis of the properties of the trajectories of individual stars to the study of collective motion of stars. A discussion of the dynamics of correlations and wave processes in such clusters is presented. The mechanisms of the dynamic evolution of OSCs, the gravitational instability of OSC nuclei, the spectra of frequencies and wavenumbers for oscillations of numerical models of OSCs, astrophysical applications of the results of studies of the dynamics of OSCs are considered.

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Baer, Tomas, and William L. Hase. Unimolecular Reaction Dynamics. Oxford University Press, 1996. http://dx.doi.org/10.1093/oso/9780195074949.001.0001.

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This book provides a penetrating and comprehensive description of energy selected reactions from a theoretical as well as experimental view. Three major aspects of unimolecular reactions involving the preparation of the reactants in selected energy states, the rate of dissociation of the activated molecule, and the partitioning of the excess energy among the final products, are fully discussed with the aid of 175 illustrations and over 1,000 references, most from the recent literature. Examples of both neutral and ionic reactions are presented. Many of the difficult topics are discussed at sev

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Book chapters on the topic "Galaxy clusters/dynamics study"

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Džanović, Dajana, R. M. Sharples, A. J. Benson, and C. S. Frenk. "Quantitative Study of Galaxy Morphology." In Galaxy Evolution in Groups and Clusters. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0107-6_10.

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Godwin, P. J. "Core and Tidal Radii of the Carina Dwarf Spheroidal Galaxy from UK Schmidt Telescope Plates." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_9.

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van Leeuwen, Floor. "A Proper Motion Study of the Pleiades Cluster." In Dynamics of Star Clusters. Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5335-2_55.

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Massobrio, Carlo, and Brahim Nacer. "Collisional dynamics of Ag19 on Pd(100): a molecular dynamics study." In Small Particles and Inorganic Clusters. Springer Berlin Heidelberg, 1997. http://dx.doi.org/10.1007/978-3-642-60854-4_126.

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Wang, Q., M. P. Iñiguez, and J. A. Alonso. "Molecular dynamics study of A18B Lennard-Jones clusters." In Atomic and Nuclear Clusters. Springer Berlin Heidelberg, 1995. http://dx.doi.org/10.1007/978-3-642-79696-8_76.

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Blaisten-Barojas, Estela, and D. Levesque. "A Molecular Dynamics Study of Silicon Clusters." In Physics and Chemistry of Small Clusters. Springer US, 1987. http://dx.doi.org/10.1007/978-1-4757-0357-3_25.

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Lugger, Phyllis M. "An Investigation of the Radial Dependence of the Galaxy Luminosity Function in Abell Clusters." In Structure and Dynamics of Elliptical Galaxies. Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3971-4_72.

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Mathieu, Robert D. "$$\lambda $$ λ Ori: A Case Study in Star Formation." In Dynamics of Young Star Clusters and Associations. Springer Berlin Heidelberg, 2015. http://dx.doi.org/10.1007/978-3-662-47290-3_11.

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Richert, R., S. Y. Goldberg, B. Fainberg, and D. Huppert. "Ultrafast Solvation Dynamics by Degenerate Four Wave Mixing: A Theoretical and Experimental Study." In Reaction Dynamics in Clusters and Condensed Phases. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0786-0_17.

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Zhao, Jijun. "The Coordination and Dynamic Analysis of Industrial Clusters: A Multi-agent Simulation Study." In Optimization and Dynamics with Their Applications. Springer Singapore, 2017. http://dx.doi.org/10.1007/978-981-10-4214-0_7.

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Conference papers on the topic "Galaxy clusters/dynamics study"

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Battistelli, Elia. "Sunyaev Zel’dovich study of filamentary structuresbetween galaxy clusters." In Multifrequency Behaviour of High Energy Cosmic Sources - XIII. Sissa Medialab, 2020. http://dx.doi.org/10.22323/1.362.0008.

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LOBO, C., and M. SEROTE ROOS. "STUDY OF THREE GALAXY CLUSTERS AT INTERMEDIATE REDSHIFTS." In Proceedings of the 15th Portuguese National Meeting. WORLD SCIENTIFIC, 2006. http://dx.doi.org/10.1142/9789812773067_0013.

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Ferrari, C., Arwa Dabbech, Oleg Smirnov, et al. "Non-thermal emission from galaxy clusters: feasibility study with SKA." In Advancing Astrophysics with the Square Kilometre Array. Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.215.0075.

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FAMAEY, B., G. W. ANGUS, G. GENTILE, H. Y. SHAN, and H. S. ZHAO. "THE WEDDING OF MODIFIED DYNAMICS AND NON-EXOTIC DARK MATTER IN GALAXY CLUSTERS." In Proceedings of the 6th International Heidelberg Conference. WORLD SCIENTIFIC, 2008. http://dx.doi.org/10.1142/9789812814357_0039.

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Giacintucci, S., J. M. Vrtilek, E. O’Sullivan, et al. "AGN Feedback in Galaxy Groups: A Joint GMRT∕X-ray Study." In THE MONSTER’S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS. AIP, 2009. http://dx.doi.org/10.1063/1.3293043.

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DING, FENG, KIM BOLTON, and ARNE ROSÉN. "MOLECULAR DYNAMICS STUDY OF IRON CLUSTER COALESCENCE AT SUB-MELTING POINT TEMPERATURES." In Clusters and Nano-Assemblies - Physical and Biological Systems. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701879_0008.

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Victor Ribeiro de Jesus, João, and Rodrigo Lyra. "Um Estudo Sobre Identificação de Aglomerados de Galáxias." In Computer on the Beach. Universidade do Vale do Itajaí, 2020. http://dx.doi.org/10.14210/cotb.v11n1.p048-049.

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Galaxy clusters are fundamental blocks of our universe, like stars and galaxies. The study of galaxy clusters has shown complexity due to a large number of stars superimposed on these clusters, which emit light and block the clear optical band visualization of the phenomenon. In this paper, we present the implementation of an algorithm capable of classifying and remove the stars of spatial images. The purpose is to improve not only the existing studies around galaxy clusters but also to assist the developing in astronomic researches with available treated spatial images.

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Suzuki, Masaaki, Hiroshi Okuda, and Genki Yagawa. "Large-Scale Biomolecular Dynamics Using SMP Clusters." In 12th International Conference on Nuclear Engineering. ASMEDC, 2004. http://dx.doi.org/10.1115/icone12-49573.

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The authors have applied Message Passing Interface (MPI) / OpenMP hybrid parallel programming model to molecular dynamics (MD) method for simulating a protein structure on a symmetric multiprocessor (SMP) cluster architecture. In that architecture, it can be expected that the hybrid parallel programming model, which uses the message passing library such as MPI for inter-SMP node communication and the loop directives such as OpenMP for intra-SMP node parallelization, is the most effective one. In this study, the parallel performance of the hybrid style has been compared with that of conventiona

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Chen, Min. "Characteristics of Helium Diffusion Trajectory: A Molecular Dynamics Study." In 2013 21st International Conference on Nuclear Engineering. American Society of Mechanical Engineers, 2013. http://dx.doi.org/10.1115/icone21-16466.

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Molecular dynamics (MD) are employed to explore the features of Helium atom and He clusters diffusion in titanium at the temperatures between room temperature and 667k. The results demonstrate that the frequency for Helium atom jumping from site to site increases with the increasing temperature. Another important feature is that the diffusion of a He atom and a He trimer is a layered structure. The difference is that the trajectory of a He atom is between two Ti atom layers of (001) planes, and the trajectory of a He trimer is overlapped with the Ti atom layers of (001) plane. Meanwhile, it is

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Desfrançois, C., and J. P. Schermann. "A collisional approach for the study of electron solvation in water and ammonia clusters and autodetachment of solvated molecular anions." In Ultrafast reaction dynamics and solvent effects. AIP, 1994. http://dx.doi.org/10.1063/1.45413.

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