Gotowe bibliografie tematyczne / Clusters of galaxies

Spis treści

  1. Artykuły w czasopismach
  2. Rozprawy doktorskie
  3. Książki
  4. Części książek
  5. Streszczenia konferencji
  6. Raporty organizacyjne

Gotowa bibliografia na temat „Clusters of galaxies”

Autor: Grafiati
Data publikacji: 4 czerwca 2021
Data aktualizacji: 18 maja 2024

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Artykuły w czasopismach na temat "Clusters of galaxies"

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Jeon, Seyoung, Sukyoung K. Yi, Yohan Dubois, Aeree Chung, Julien Devriendt, San Han, Ryan A. Jackson, Taysun Kimm, Christophe Pichon, and Jinsu Rhee. "Star Formation History and Transition Epoch of Cluster Galaxies Based on the Horizon-AGN Simulation." Astrophysical Journal 941, no. 1 (December 1, 2022): 5. http://dx.doi.org/10.3847/1538-4357/ac9d8c.

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Abstract Cluster galaxies exhibit substantially lower star formation rates than field galaxies today, but it is conceivable that clusters were sites of more active star formation in the early universe. Herein, we present an interpretation of the star formation history (SFH) of group/cluster galaxies based on the large-scale cosmological hydrodynamic simulation, Horizon-AGN. We find that massive galaxies in general have small values of e-folding timescales of star formation decay (i.e., “mass quenching”) regardless of their environment, while low-mass galaxies exhibit prominent environmental de
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Kuchner, Ulrike, Roan Haggar, Alfonso Aragón-Salamanca, Frazer R. Pearce, Meghan E. Gray, Agustín Rost, Weiguang Cui, Alexander Knebe, and Gustavo Yepes. "An inventory of galaxies in cosmic filaments feeding galaxy clusters: galaxy groups, backsplash galaxies, and pristine galaxies." Monthly Notices of the Royal Astronomical Society 510, no. 1 (November 27, 2021): 581–92. http://dx.doi.org/10.1093/mnras/stab3419.

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ABSTRACT Galaxy clusters grow by accreting galaxies from the field and along filaments of the cosmic web. As galaxies are accreted they are affected by their local environment before they enter (pre-processing), and traverse the cluster potential. Observations that aim to constrain pre-processing are challenging to interpret because filaments comprise a heterogeneous range of environments including groups of galaxies embedded within them and backsplash galaxies that contain a record of their previous passage through the cluster. This motivates using modern cosmological simulations to dissect t
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Aguerri, J. A. L., M. Girardi, I. Agulli, A. Negri, C. Dalla Vecchia, and L. Domínguez Palmero. "Deep spectroscopy in nearby galaxy clusters – V. The Perseus cluster." Monthly Notices of the Royal Astronomical Society 494, no. 2 (March 24, 2020): 1681–92. http://dx.doi.org/10.1093/mnras/staa800.

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ABSTRACT Dwarfs are the largest population of galaxies in number in the nearby Universe. Deep spectroscopic data are still missing to obtain a better understanding of their formation and evolution processes. This study shows the results obtained from a spectroscopic campaign in the Perseus cluster. We have obtained 963 new galaxy spectra. We have measured the recessional velocity of the galaxies by using a cross-correlation technique. These data have been used to obtain the cluster membership, the dynamics of the galaxies, and the spectroscopic luminosity function (LF) of the cluster. The clus
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Pallero, Diego, Facundo A. Gómez, Nelson D. Padilla, Yannick M. Bahé, Cristian A. Vega-Martínez, and S. Torres-Flores. "Too dense to go through: the role of low-mass clusters in the pre-processing of satellite galaxies." Monthly Notices of the Royal Astronomical Society 511, no. 3 (November 17, 2021): 3210–27. http://dx.doi.org/10.1093/mnras/stab3318.

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ABSTRACT We study the evolution of satellite galaxies in clusters of the c-eagle simulations, a suite of 30 high-resolution cosmological hydrodynamical zoom-in simulations based on the eagle code. We find that the majority of galaxies that are quenched at z = 0 (≳80${{\ \rm per\ cent}}$) reached this state in a dense environment (log10M200[M⊙] ≥13.5). At low redshift, regardless of the final cluster mass, galaxies appear to reach their quenching state in low-mass clusters. Moreover, galaxies quenched inside the cluster that they reside in at z = 0 are the dominant population in low-mass cluste
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Teague, P. F., and D. Carter. "Modelling Clusters of Galaxies." Publications of the Astronomical Society of Australia 6, no. 2 (1985): 198–202. http://dx.doi.org/10.1017/s1323358000018087.

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AbstractThorough investigation of clusters of galaxies involves the complete modelling of their dynamics and structure. Presented here is a description of such a substantial project utilizing a sample of several rich southern clusters of galaxies. Incorporating results from radial velocity analyses of cluster galaxies and X-ray images of the clusters into rigorously constructed models of the cluster potential well and atmosphere will enable the dynamics, structure and evolution of clusters to be tied down.
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Bogdán, Ákos, Lorenzo Lovisari, Patrick Ogle, Orsolya E. Kovács, Thomas Jarrett, Christine Jones, William R. Forman, and Lauranne Lanz. "Detection of a Superluminous Spiral Galaxy in the Heart of a Massive Galaxy Cluster." Astrophysical Journal 930, no. 2 (May 1, 2022): 138. http://dx.doi.org/10.3847/1538-4357/ac62cd.

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Abstract It is well established that brightest cluster galaxies (BCGs), residing in the centers of galaxy clusters, are typically massive and quenched galaxies with cD or elliptical morphology. An optical survey suggested that an exotic galaxy population, superluminous spiral and lenticular galaxies, could be the BCGs of some galaxy clusters. Because the cluster membership and the centroid of a cluster cannot be accurately determined based solely on optical data, we followed up a sample of superluminous disk galaxies and their environments using XMM-Newton X-ray observations. Specifically, we
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Godłowski, W., and F. Baier. "Galaxy Orientation in Some Abell Clusters." Symposium - International Astronomical Union 186 (1999): 410. http://dx.doi.org/10.1017/s0074180900113245.

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We analyze a sample of galaxies in a region of three rich Abell Clusters. The data are taken from the Edinburgh Catalogue of the cluster. First, we divide the whole cluster area into different parts according to the assumed subclusters. Now we can find the position angles of the cluster and subclusters. We find strong evidence that the position angles of galaxies within our clusters are aligned to a large extent. For the cluster A754, position angles of galaxies tend to be perpendicular to the direction of the position angle of the cluster. Consequently, the angular momentum of galaxies are pr
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Anders, Peter, Uta Fritze –. v. Alvensleben, and Richard de Grijs. "Young Star Clusters: Progenitors of Globular Clusters!?" Highlights of Astronomy 13 (2005): 366–68. http://dx.doi.org/10.1017/s1539299600015987.

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AbstractStar cluster formation is a major mode of star formation in the extreme conditions of interacting galaxies and violent starbursts. Young clusters are observed to form in a variety of such galaxies, a substantial number resembling the progenitors of globular clusters in mass and size, but with significantly enhanced metallicity. From studies of the metal-poor and metal-rich star cluster populations of galaxies, we can therefore learn about the violent star formation history of these galaxies, and eventually about galaxy formation and evolution. We present a new set of evolutionary synth
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Maier, C., C. P. Haines, and B. L. Ziegler. "Star-formation quenching of cluster galaxies as traced by metallicity and presence of active galactic nuclei, and galactic conformity." Astronomy & Astrophysics 658 (February 2022): A190. http://dx.doi.org/10.1051/0004-6361/202141498.

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Aims. We strive to explore the differences in the properties and quenching processes of satellite galaxies in a sample of massive clusters with passive and star-forming (SF) brightest cluster galaxies (BCGs). One aim is to investigate galactic conformity effects, manifested in a correlation between the fraction of satellite galaxies that halted star formation and the state of star formation in the central galaxy. Methods. We explored 18 clusters from the Local Cluster Substructure Survey at 0.15 < z < 0.26, using spectra from the Arizona Cluster Redshift Survey Hectospec survey of about
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Larsen, Søren S. "Open, Massive and Globular Clusters — Part of the Same Family?" Symposium - International Astronomical Union 207 (2002): 421–27. http://dx.doi.org/10.1017/s0074180900224133.

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Populations of young star clusters show significant differences even among “normal” disk galaxies. In this contribution I discuss how properties of young cluster systems are related to those of their host galaxies, based on a recent study of clusters in a sample of 22 nearby spiral galaxies. Luminous young clusters similar to the “super” star clusters observed in starbursts and mergers exist in several of these galaxies, and it is found that the luminosity of the brightest star cluster as well as the specific luminosity of the cluster systems both correlate well with the host galaxy star forma
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Rozprawy doktorskie na temat "Clusters of galaxies"

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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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Jeltema, Tesla Erin. "Cosmology with clusters of galaxies : high-redshift clusters and the evolution of cluster substructure." Thesis, Massachusetts Institute of Technology, 2004. http://hdl.handle.net/1721.1/28372.

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Thesis (Ph. D.)--Massachusetts Institute of Technology, Dept. of Physics, 2004.<br>Includes bibliographical references (p. 85).<br>Clusters of galaxies have become an important cosmological tool, yet we do not un-erstand many aspects of their formation and development. In this thesis, I pursue two projects aimed at using clusters to constrain cosmology and better understanding cluster evolution. First, I examine the Chandra observation of MS1054-0321. MS1054-0321 is the highest redshift cluster in the Einstein Medium Sensitivity Survey (EMSS), and it was one of the first high-redshift clusters
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De, Lucia Gabriella. "Evolution of Galaxies in Clusters." Diss., lmu, 2004. http://nbn-resolving.de/urn:nbn:de:bvb:19-25762.

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White, David Allen. "The multiphase medium of elliptical galaxies and clusters of galaxies." Thesis, University of Cambridge, 1992. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.240155.

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Piffaretti, Rocco. "Faraday rotation in clusters of galaxies." Zürich : ETH, Eidgenössische Technische Hochschule, 2000. http://e-collection.ethbib.ethz.ch/show?type=dipl&nr=17.

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Reblinsky, Katrin. "Projection effects in clusters of galaxies." Diss., lmu, 2000. http://nbn-resolving.de/urn:nbn:de:bvb:19-4153.

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Mora, Marcelo D. "Star clusters in unperturbed spiral galaxies." Diss., lmu, 2008. http://nbn-resolving.de/urn:nbn:de:bvb:19-92728.

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MacLaren, Ian. "Studies of distant clusters of galaxies." Thesis, Durham University, 1987. http://etheses.dur.ac.uk/6891/.

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A technique of constructing crude, low-resolution Spectral Energy Distributions (SEDs) for galaxies in distant clusters, using a set of intermediate bandwidth filters and a CCD detector, is developed which is capable of redressing many of the problems which have previously beset work in this field. The technique has been used to study galaxies in the distant clusters 0016+16 (z = 0.54) and Abell 370 (z = 0.37).These SEDs are then used to individually classify each object in the CCD field, ascribing both an estimated redshift and a galaxy type. The SEDs have been extended into the rest-frame ul
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Basson, J. F. "Cold gas in clusters of galaxies." Thesis, University of Cambridge, 2003. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.596456.

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The intracluster gas has only been fully explored in the last decade or so with the launch of the <i>ROSAT</i> satellite in 1990, and more recently the <i>Chandra</i> and <i>XMM-Newton</i> satellites in 1999. The data obtained from these X-ray telescopes has provided significant information about the intracluster medium. In this thesis, a theoretical and numerical study of the nature of the ICM is undertaken. In particular the formation and influence of cold gas clouds and the effects of powerful FR-II radio sources are considered. Clusters are modelled as a multi-phase cooling gas in a dark-m
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Moore, Ben. "Groups, clusters and superclusters of galaxies." Thesis, Durham University, 1991. http://etheses.dur.ac.uk/6091/.

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Galaxies are observed in a diverse range of associations. Understanding the dynamical, statistical and clustering properties of aggregations of galaxies forms the main body of this thesis. On the smallest scale, we use a model for the Local Group to study the formation of a typical galaxy system and to understand the mass distribution within the Local Group. Our model is a binary system excised from numerical simulation of a Universe dominated by cold dark matter which has similar radial velocity and separation as M31 and the Milky Way. We find that the timing argument provides a reliable meth
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Książki na temat "Clusters of galaxies"

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Kaastra, Jelle, ed. Clusters of Galaxies. New York, NY: Springer New York, 2008. http://dx.doi.org/10.1007/978-0-387-78875-3.

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Galaxies. Cambridge, Mass: Harvard University Press, 1986.

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Stars, clusters, and galaxies. New York, NY: J. Messner, 1992.

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Ip, Peter Shun Sang. Binary galaxies in clusters. Toronto: University of Toronto, Dept. of Astronomy, 1994.

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Stars, clusters, and galaxies. New York, NY: Scholastic Inc., 1992.

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Hobbs, Ian Stuart. The motions of galaxies in clusters of galaxies. Birmingham: University of Birmingham, 1997.

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Richtler, Tom, and Søren Larsen, eds. Globular Clusters - Guides to Galaxies. Berlin, Heidelberg: Springer Berlin Heidelberg, 2009. http://dx.doi.org/10.1007/978-3-540-76961-3.

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Fabian, A. C., ed. Clusters and Superclusters of Galaxies. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2482-9.

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NATO, Advanced Study Institute on Clusters and Superclusters of Galaxies (1991 Cambridge England). Clusters and superclusters of galaxies. Dordrecht: Kluwer Academic Publishers, 1992.

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Fabian, A. C. Clusters and Superclusters of Galaxies. Dordrecht: Springer Netherlands, 1992.

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Części książek na temat "Clusters of galaxies"

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Parker, Barry. "Clusters and Superclusters." In Colliding Galaxies, 237–55. Boston, MA: Springer US, 1990. http://dx.doi.org/10.1007/978-1-4899-3348-5_12.

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Contopoulos, Georgios, and Dimitrios Kotsakis. "Galaxies and Clusters of Galaxies." In Cosmology, 32–61. Berlin, Heidelberg: Springer Berlin Heidelberg, 1987. http://dx.doi.org/10.1007/978-3-642-71464-1_3.

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Unsöld, Albrecht, and Bodo Baschek. "Galaxies and Clusters of Galaxies." In The New Cosmos, 402–67. Berlin, Heidelberg: Springer Berlin Heidelberg, 2002. http://dx.doi.org/10.1007/978-3-662-04356-1_12.

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Chincarini, Guido. "Clusters of Galaxies." In Astrophysics and Space Science Library, 217–25. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2919-7_27.

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Bower, Richard. "Clusters of Galaxies." In Planets, Stars and Stellar Systems, 265–303. Dordrecht: Springer Netherlands, 2013. http://dx.doi.org/10.1007/978-94-007-5609-0_6.

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BÖhringer, H. "Clusters of Galaxies." In Astrophysics and Space Science Library, 359–68. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-0794-5_36.

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Mushotzky, Richard. "Clusters of galaxies." In The Century of Space Science, 473–98. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0320-9_21.

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Longair, Malcolm S. "Clusters of Galaxies." In Astronomy and Astrophysics Library, 71–105. Berlin, Heidelberg: Springer Berlin Heidelberg, 1998. http://dx.doi.org/10.1007/978-3-662-03571-9_4.

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Takase, Bunshiro, Keiichi Kodaira, and Sadanori Okamura. "Clusters of Galaxies." In An Atlas of Selected Galaxies, 16–20. London: Routledge, 2023. http://dx.doi.org/10.1201/9781315137216-9.

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Takase, Bunshiro, Keiichi Kodaira, and Sadanori Okamura. "Clusters of Galaxies." In An Atlas of Selected Galaxies, 64–70. London: Routledge, 2023. http://dx.doi.org/10.1201/9781315137216-18.

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Streszczenia konferencji na temat "Clusters of galaxies"

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Kopylova, F., and A. Kopylov. "Study of groups/clusters of galaxies with the SDSS." In ASTRONOMY AT THE EPOCH OF MULTIMESSENGER STUDIES. Proceedings of the VAK-2021 conference, Aug 23–28, 2021. Crossref, 2022. http://dx.doi.org/10.51194/vak2021.2022.1.1.148.

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For a large sample of groups/clusters of galaxies (N =185), we obtained the scaling relations among of their photometricaland dynamical parameters. We find:0.77±0.011. that in the virialized regions of the galaxy systems the total luminosity increase with mass L K ∝ M 200(M K &lt;−21. m 0);2. that the new halo boundary of the galaxy systems corresponds to the splashback radius R sp . These radius is definedby the observed intergrated distribution of the number of galaxies as a function of the angular distance from thegroup/cluster center squared;3. that the fraction of galaxies with quenched sta
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Chincarini, Guido. "Clusters of Galaxies: A Commentary." In A Festschrift in Honor of Ricardo Giacconi. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812792174_0012.

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Bahcall, Neta A. "Cosmology with Clusters of Galaxies." In Proceedings of Nobel Symposium 109. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812810434_0003.

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DONAHUE, M. "COSMOLOGY WITH CLUSTERS OF GALAXIES." In Proceedings of the 32nd Coral Gables Conference. WORLD SCIENTIFIC, 2005. http://dx.doi.org/10.1142/9789812701992_0018.

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Poggianti, Bianca. "Evolution of galaxies in clusters." In Baryons in Dark Matter Halos. Trieste, Italy: Sissa Medialab, 2004. http://dx.doi.org/10.22323/1.014.0104.

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Mushotzky, Richard F. "The missing mass in clusters of galaxies and elliptical galaxies." In After the first three minutes. AIP, 1991. http://dx.doi.org/10.1063/1.40402.

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CAVALIERE, A. "CLUSTERS OF GALAXIES IN X-RAYS." In A Festschrift in Honor of Ricardo Giacconi. WORLD SCIENTIFIC, 2000. http://dx.doi.org/10.1142/9789812792174_0010.

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FABIAN, A. C., and S. W. ALLEN. "X-RAYS FROM CLUSTERS OF GALAXIES." In Proceedings of the XXI Symposium on Relativistic Astrophysics. WORLD SCIENTIFIC, 2003. http://dx.doi.org/10.1142/9789812704009_0018.

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Ferrari, L., D. Bagliani, A. Bardi, E. Battistelli, M. Birkinshaw, S. Colafrancesco, A. Conte, et al. "Spectroscopic Active Galaxies and Clusters Explorer." In THE THIRTEENTH INTERNATIONAL WORKSHOP ON LOW TEMPERATURE DETECTORS—LTD13. AIP, 2009. http://dx.doi.org/10.1063/1.3292383.

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Garilli, Bianca, Dario Maccagni, Luis Carrasco, and Elsa Recillas. "Photometric properties of clusters of galaxies." In Dark matter. AIP, 1995. http://dx.doi.org/10.1063/1.48328.

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Raporty organizacyjne na temat "Clusters of galaxies"

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Blanton, Elizabeth L., T. E. Clarke, Craig L. Sarazin, Scott W. Randall, and Brian R. McNamara. AGN Feedback in Clusters of Galaxies. Fort Belvoir, VA: Defense Technical Information Center, January 2010. http://dx.doi.org/10.21236/ada520956.

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Rykoff, E. S. The L_X-M relation of Clusters of Galaxies. Office of Scientific and Technical Information (OSTI), May 2008. http://dx.doi.org/10.2172/928354.

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Zhang, Yuanyuan. Looking Wider and Further: The Evolution of Galaxies Inside Galaxy Clusters. Office of Scientific and Technical Information (OSTI), January 2016. http://dx.doi.org/10.2172/1248222.

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Press, W. H. (Astrophysics of binary stars, Seyfert galaxies, quasars, and globular clusters. Final technical report. Office of Scientific and Technical Information (OSTI), March 1985. http://dx.doi.org/10.2172/6429223.

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Werner, Norbert, J. de Plaa, J. S. Kaastra, Jacco Vink, J. A. M. Bleeker, T. Tamura, J. R. Peterson, and F. Verbunt. XMM-Newton Spectroscopy of the Cluster of Galaxies 2a 0335+096. Office of Scientific and Technical Information (OSTI), January 2006. http://dx.doi.org/10.2172/878003.

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Miley, G., C. Carilli, G. B. Taylor, C. de Breuck, and A. Cohen. High Redshift Radio Galaxies: Laboratories for Massive Galaxy and Cluster Formation in the Early Universe. Fort Belvoir, VA: Defense Technical Information Center, January 2010. http://dx.doi.org/10.21236/ada520904.

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