Relevant bibliographies by topics / Galaxy formation clusters

Contents

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

Academic literature on the topic 'Galaxy formation clusters'

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 'Galaxy formation clusters.'

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 "Galaxy formation clusters"

1

Larson, Richard B. "Galaxy Formation and Cluster Formation." Symposium - International Astronomical Union 126 (1988): 311–21. http://dx.doi.org/10.1017/s007418090004256x.

Full text
Abstract:
A primary motivation for studying globular clusters is that, as the oldest known galactic fossils, they trace the earliest stages of galactic evolution; indeed, they may hold the key to understanding galaxy formation. Thus it is clearly of great importance to learn how to read the fossil record. To do this, we need to understand something about how the globular clusters themselves formed. Were they the first bound objects to form, or did they form in larger pre-existing systems of which they are just small surviving fragments? If the latter, what were the prehistoric cluster-forming systems li
APA, Harvard, Vancouver, ISO, and other styles
2

Robertson, Andrew. "The galaxy–galaxy strong lensing cross-sections of simulated ΛCDM galaxy clusters". Monthly Notices of the Royal Astronomical Society: Letters 504, № 1 (2021): L7—L11. http://dx.doi.org/10.1093/mnrasl/slab028.

Full text
Abstract:
ABSTRACT We investigate a recent claim that observed galaxy clusters produce an order of magnitude more galaxy–galaxy strong lensing (GGSL) than simulated clusters in a Λ cold dark matter (CDM) cosmology. We take galaxy clusters from the c-eagle hydrodynamical simulations and calculate the expected amount of GGSL for sources placed behind the clusters at different redshifts. The probability of a source lensed by one of the most massive c-eagle clusters being multiply imaged by an individual cluster member is in good agreement with that inferred for observed clusters. We show that numerically c
APA, Harvard, Vancouver, ISO, and other styles
3

Blau, Steven K. "Galaxy clusters in formation." Physics Today 68, no. 6 (2015): 20. http://dx.doi.org/10.1063/pt.3.2807.

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

Kravtsov, Andrey V., and Stefano Borgani. "Formation of Galaxy Clusters." Annual Review of Astronomy and Astrophysics 50, no. 1 (2012): 353–409. http://dx.doi.org/10.1146/annurev-astro-081811-125502.

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

Neumayer, Nadine. "Nuclear Star Clusters." Proceedings of the International Astronomical Union 12, S316 (2015): 84–90. http://dx.doi.org/10.1017/s1743921316007018.

Full text
Abstract:
AbstractThe centers of galaxies host two distinct, compact components: massive black holes and nuclear star clusters. Nuclear star clusters are the densest stellar systems in the universe, with masses of ~ 107M⊙and sizes of ~ 5pc. They are almost ubiquitous at the centres of nearby galaxies with masses similar to, or lower than the Milky Way. Their occurrence both in spirals and dwarf elliptical galaxies appears to be a strong function of total galaxy light or mass. Nucleation fractions are up to 100% for total galaxy magnitudes of MB= −19mag or total galaxy luminosities of about LB= 1010L⊙and
APA, Harvard, Vancouver, ISO, and other styles
6

van den Bergh, S. "Star clusters in the Magellanic Clouds." Symposium - International Astronomical Union 148 (1991): 161–64. http://dx.doi.org/10.1017/s0074180900200259.

Full text
Abstract:
Star clusters in the Magellanic Clouds (MCs) differ from those in the Galaxy in a number of respects: (1) the Clouds contain a class of populous open clusters that has no Galactic counterpart; (2) Cloud clusters have systematically larger radii rh than those in the Galaxy; (3) clusters of all ages in the Clouds are, on average, more flattened than those in the Galaxy. In the Large Magellanic Cloud (LMC) there appear to have been two distinct epochs of cluster formation. LMC globulars have ages of 12-15 Gyr, whereas most populous open clusters have ages <5 Gyr. No such dichotomy is observed
APA, Harvard, Vancouver, ISO, and other styles
7

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.

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

Henriksen, Mark J., and Prajwal Panda. "Exploiting Machine Learning and Disequilibrium in Galaxy Clusters to Obtain a Mass Profile." Astrophysical Journal Letters 961, no. 2 (2024): L36. http://dx.doi.org/10.3847/2041-8213/ad1ede.

Full text
Abstract:
Abstract We use 3D k-means clustering to characterize galaxy substructure in the A2146 cluster of galaxies (z = 0.2343). This method objectively characterizes the cluster’s substructure using projected position and velocity data for 67 galaxies within a 2.305 Mpc circular region centered on the cluster's optical center. The optimal number of substructures is found to be four. Four distinct substructures with rms velocity typical of galaxy groups or low-mass subclusters, when compared to cosmological simulations of galaxy cluster formation, suggest that A2146 is in the early stages of formation
APA, Harvard, Vancouver, ISO, and other styles
9

Lee, Seong-Kook, Myungshin Im, Eunhee Ko, et al. "Star-formation Property of High Redshift Galaxies in Clusters: Perceptive View from Observation and Simulation." Proceedings of the International Astronomical Union 17, S373 (2021): 260–63. http://dx.doi.org/10.1017/s1743921322004409.

Full text
Abstract:
AbstractThe evolution of star formation properties of galaxies depends on the environment where galaxies reside, and generally star formation of galaxies in dense environment decreases more quickly. Interestingly, the star formation property of high-redshift galaxies clusters vary largely even though they are at similar redshift. We have found that the large-scale environment surrounding each galaxy cluster can contribute to make this cluster-by-cluster variation. This correlation is found in the results from observational data as well as in the simulations of galaxy formation. We suggest the
APA, Harvard, Vancouver, ISO, and other styles
10

Danieli, Shany, Pieter van Dokkum, Sebastian Trujillo-Gomez, et al. "NGC 5846-UDG1: A Galaxy Formed Mostly by Star Formation in Massive, Extremely Dense Clumps of Gas." Astrophysical Journal Letters 927, no. 2 (2022): L28. http://dx.doi.org/10.3847/2041-8213/ac590a.

Full text
Abstract:
Abstract It has been shown that ultra-diffuse galaxies (UDGs) have higher specific frequencies of globular clusters, on average, than other dwarf galaxies with similar luminosities. The UDG NGC 5846-UDG1 is among the most extreme examples of globular cluster–rich galaxies found so far. Here we present new Hubble Space Telescope observations and analysis of this galaxy and its globular cluster system. We find that NGC 5846-UDG1 hosts 54 ± 9 globular clusters, three to four times more than any previously known galaxy with a similar luminosity and higher than reported in previous studies. With a
APA, Harvard, Vancouver, ISO, and other styles
More sources

Dissertations / Theses on the topic "Galaxy formation clusters"

1

Beasley, Michael Andrew. "Globular clusters as probes of galaxy formation." Thesis, Durham University, 2001. http://etheses.dur.ac.uk/4949/.

Full text
Abstract:
Observations and analysis of globular cluster systems associated with three galaxy types are presented. Spectroscopy of globular cluster (GC) candidates in the Sculptor spirals NGC 253 and NGC 55 has identified 15 GCs in these galaxies. This spectroscopic sample, combined with plate scans, indicates total GC populations consistent with that expected for their luminosity and morphological type. From these data, we define new GC samples for spectroscopy. Radial velocities of 87 GCs in the Virgo elliptical NGC 4472 have been obtained, yielding data for 144 GCs when combined with previous studies.
APA, Harvard, Vancouver, ISO, and other styles
2

Contini, Emanuele. "Galaxy populations in clusters and proto-clusters." Doctoral thesis, Università degli studi di Trieste, 2014. http://hdl.handle.net/10077/9964.

Full text
Abstract:
2012/2013<br>The aim of my Thesis is to explore the physical properties of the galaxy population in clusters and proto-clusters. A large number of physical processes plays an important role in the formation and evolution of galaxies: cooling, that allows the condensation of gas in the centre of dark matter haloes; star formation, that converts cold gas in stars; feedback from Active Galactic Nuclei (AGN), that prevents the gas in the central regions of haloes from "over-cooling"; feedback from Supernovae, which liberates energy in the surrounding, mixing the gas and enriching it with hea
APA, Harvard, Vancouver, ISO, and other styles
3

Finn, Rose A. "Star-formation rates of high-redshift galaxy clusters." Diss., The University of Arizona, 2003. http://hdl.handle.net/10150/289932.

Full text
Abstract:
In this thesis, we take the first step toward building a star-formation limited sample of z ∼ 0.8 cluster galaxies with the goal of understanding the physical processes that affect star formation within the cluster environment. We present Hα narrow-band imaging results for four z ∼ 0.8 clusters. We reach 3σ star-formation rate (SFR) limits of ≤ 0.3 h⁻²₁₀₀M(⊙) yr⁻¹, demonstrating that near-infrared, narrow-band imaging centered on the observed wavelength of Hα is a powerful technique for sampling the entire Halpha luminosity function even at relatively high redshifts where Halpha emission moves
APA, Harvard, Vancouver, ISO, and other styles
4

Ruggiero, Rafael. "Galaxy Evolution in Clusters." Universidade de São Paulo, 2018. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-14022019-140755/.

Full text
Abstract:
In this thesis, we aim to further elucidate the phenomenon of galaxy evolution in the environment of galaxy clusters using the methodology of numerical simulations. For that, we have developed hydrodynamic models in which idealized gas-rich galaxies move within the ICM of idealized galaxy clusters, allowing us to probe in a detailed and controlled manner their evolution in this extreme environment. The main code used in our simulations is RAMSES, and our results concern the changes in gas composition, star formation rate, luminosity and color of infalling galaxies. Additionally to processes ta
APA, Harvard, Vancouver, ISO, and other styles
5

Steel, James. "Surface photometry of early-type galaxies in rich clusters." Thesis, Durham University, 1998. http://etheses.dur.ac.uk/4868/.

Full text
Abstract:
This thesis investigates the morphology of early-type galaxies in two rich clusters using 2D surface photometry. In particular, the amount of light in the 'disk' component is focussed upon, as the presence of a disk is the main morphological criterion in distinguishing between the traditional 'elliptical' and 'S0' classes. Extensive and photometric E-band CCD observations of continuous areas of the Coma and Abell 1367 clusters were obtained at the 2.5 m Isaac Newton telescope, La Palma during March 1994. A subset of this large data-set has been used in this study, comprising a magnitude-limite
APA, Harvard, Vancouver, ISO, and other styles
6

Tyler, Krystal D. "Star Formation and Galaxy Evolution in Different Environments, from the Field to Massive Clusters." Diss., The University of Arizona, 2012. http://hdl.handle.net/10150/265395.

Full text
Abstract:
This thesis focuses on how a galaxy's environment affects its star formation, from the galactic environment of the most luminous IR galaxies in the universe to groups and massive clusters of galaxies. Initially, we studied a class of high-redshift galaxies with extremely red optical-to-mid-IR colors. We used Spitzer spectra and photometry to identify whether the IR outputs of these objects are dominated by AGNs or star formation. In accordance with the expectation that the AGN contribution should increase with IR luminosity, we find most of our very red IR-luminous galaxies to be dominated b
APA, Harvard, Vancouver, ISO, and other styles
7

Croft, Rupert Alfred Charles. "Galaxy clusters and the formation of large-scale structures in the universe." Thesis, University of Oxford, 1995. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.308751.

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

Dias, Bruno Moreira de Souza. "Formation and evolution of globular clusters in the Galaxy and Magellanic Clouds." Universidade de São Paulo, 2014. http://www.teses.usp.br/teses/disponiveis/14/14131/tde-26082014-090039/.

Full text
Abstract:
Globular clusters are tracers of the formation and evolution of their host galaxies. Kinematics, chemical abundances, age and position of the clusters allows tracing interactions between Milky Way and surrounding galaxies and outlines their chemical enrichment history. In this thesis we analyse mid-resolution spectra of about 800 red giant stars in 51 Galactic globular clusters. It is the first time that [Fe/H] and [Mg/Fe] derived in a consistent way are published for such a huge sample of globular clusters, almost 1/3 of the total number of catalogued clusters. Our metallicities are showed to
APA, Harvard, Vancouver, ISO, and other styles
9

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.

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

Snyder, Gregory Frantz. "Modeling Spatially and Spectrally Resolved Observations to Diagnose the Formation of Elliptical Galaxies." Thesis, Harvard University, 2013. http://dissertations.umi.com/gsas.harvard:10893.

Full text
Abstract:
In extragalactic astronomy, a central challenge is that we cannot directly watch what happens to galaxies before and after they are observed. This dissertation focuses on linking predictions of galaxy time-evolution directly with observations, evaluating how interactions, mergers, and other processes affect the appearance of elliptical galaxies. The primary approach is to combine hydrodynamical simulations of galaxy formation, including all major components, with dust radiative transfer to predict their observational signatures. The current paradigm implies that a quiescent elliptical emerges
APA, Harvard, Vancouver, ISO, and other styles
More sources

Books on the topic "Galaxy formation clusters"

1

International, School of Physics "Enrico Fermi" (1991 Varenna Italy). Galaxy formation: Varenna on Lake Como, Villa Monastero, 21-31 July 1992. North-Holland, 1994.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
2

Symposium, International Astronomical Union. The central regions of the galaxy and galaxies: Proceedings of the 184th Symposium of the International Astronomical Union, held in Tokyo, Japan, August 18-22. Kluwer Academic, 1998.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
3

Symposium, International Astronomical Union. The central regions of the galaxy and galaxies: Proceedings of the 184th Symposium of the International Astronomical Union, held in Tokyo, Japan, August 18-22, 1997. Kluwer Academic, 1998.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
4

Frieswijk, Willem Freerk. Early stages of clustered star formation: Massive dark clouds throughout the galaxy. Ipskamp B.V. (printer), 2008.

Find full text
APA, Harvard, Vancouver, ISO, and other styles
5

Euro-Asian Astronomical Society, _., ed. Astronomical and Astrophysical Transactions, Vol. 32, No. 2. Cambridge Scientific Publishers, 2021. http://dx.doi.org/10.17184/eac.9781908106797.

Full text
Abstract:
This issue of Astronomical and Astrophysical Transactions comprises the papers presented at the tenth annual conference on Modern Stellar Astronomy, held in Special Astrophysical Observatory of the Russian Academy of Sciences in October 2019. The “Modern Stellar Astronomy” conferences provide a forum for Russian scientists and scientists from the former Soviet Union concerned with stellar astronomy and related topics. The program consisted of invited talks, contributed oral talks, and poster papers. There were about 110 registered participants at the meeting. The program of the 2019 conference
APA, Harvard, Vancouver, ISO, and other styles

Book chapters on the topic "Galaxy formation clusters"

1

Frenk, Carlos S. "Galaxy Clusters and the Epoch of Galaxy Formation." In The Epoch of Galaxy Formation. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0919-9_28.

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

Silk, Joseph. "Galaxy Formation in Galaxy Clusters: A Phenomenological Approach." In Cosmological Aspects of X-Ray Clusters of Galaxies. Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1022-8_31.

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

Ferrari, Chiara. "Star Formation in Merging Galaxy Clusters." In Reviews in Modern Astronomy. Wiley-VCH Verlag GmbH & Co. KGaA, 2006. http://dx.doi.org/10.1002/3527608966.ch7.

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

Yee, H. K. C., E. Ellingson, R. F. Green, and C. J. Pritchet. "Properties of Galaxy Clusters Associated with Quasars." In The Epoch of Galaxy Formation. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0919-9_21.

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

Bekenstein, Jacob D., and Eyal Maoz. "The Turnaround Epoch of Clusters of Galaxies." In The Epoch of Galaxy Formation. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0919-9_60.

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

Thomas, P. A. "Multiphase Cooling Flows and Galaxy Formation." In Cooling Flows in Clusters and Galaxies. Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2953-1_46.

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

Fang, Li-Zhi. "Structure Formation of Galaxy Clusters and Beyond." In Current Topics in Astrofundamental Physics: The Cosmic Microwave Background. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-010-0748-1_15.

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

Cimatti, Andrea. "The Formation and Evolution of Field Massive Galaxies." In Galaxy Evolution in Groups and Clusters. Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-010-0107-6_31.

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

Yee, H. K. C. "Simulations of the Visual Appearance of Galaxy Clusters at High Redshift." In The Epoch of Galaxy Formation. Springer Netherlands, 1989. http://dx.doi.org/10.1007/978-94-009-0919-9_53.

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

Röttgering, Huub, Carlos De Breuck, Emanuele Daddi, et al. "Clustering and Proto-Clusters in the Early Universe." In Multiwavelength Mapping of Galaxy Formation and Evolution. Springer Berlin Heidelberg, 2006. http://dx.doi.org/10.1007/10995020_8.

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

Conference papers on the topic "Galaxy formation clusters"

1

MILLER, NEAL A., and FRAZER N. OWEN. "THE FIR-RADIO CORRELATION IN NEARBY CLUSTERS: IMPLICATIONS FOR THE RADIO-TO-SUBMM INDEX REDSHIFT ESTIMATOR." In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0020.

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

Seth, Anil, Michele Cappellari, Nadine Neumayer, et al. "Nuclear Star Clusters & Black Holes." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458493.

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

Dokuchaev, V. I., Yu N. Eroshenko, S. G. Rubin, Victor P. Debattista, and C. C. Popescu. "Supermassive Black Hole Formation Inside Primordial Black Hole Clusters." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458495.

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

Jalali, Behrang, Markus Kissler-Patig, Karl Gebhardt, et al. "Intermediate Mass Black Holes in Galactic Globular Clusters." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458500.

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

Thomas, P. A., B. M. Henriques, Sebastian Heinz, and Eric Wilcots. "The Role of Active Galactic Nuclei in Galaxy Formation." In THE MONSTER’S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS. AIP, 2009. http://dx.doi.org/10.1063/1.3293083.

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

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.

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

Hartmann, Markus, Victor P. Debattista, Anil Seth, et al. "Structural and Kinematical Constraints on the Formation of Stellar Nuclear Clusters." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458499.

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

Short, C. J., P. A. Thomas, Sebastian Heinz, and Eric Wilcots. "Combining Semi-Analytic Models of Galaxy Formation with Simulations of Galaxy Clusters: the Need for AGN Heating." In THE MONSTER’S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS. AIP, 2009. http://dx.doi.org/10.1063/1.3293097.

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

Mathis, H. "Formation of cold fronts in mergers of massive galaxy clusters." In PLASMAS IN THE LABORATORY AND IN THE UNIVERSE: New Insights and New Challenges. AIP, 2004. http://dx.doi.org/10.1063/1.1718485.

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

Dogiel, V. A., Dmitry Chernyshov, Kwong-Sang Cheng, and Chung-Ming Ko. "Formation of non-thermal spectra of particles in galaxy clusters." In 8th INTEGRAL Workshop “The Restless Gamma-ray Universe”. Sissa Medialab, 2011. http://dx.doi.org/10.22323/1.115.0168.

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

Reports on the topic "Galaxy formation clusters"

1

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. Defense Technical Information Center, 2010. http://dx.doi.org/10.21236/ada520904.

Full text
APA, Harvard, Vancouver, ISO, and other styles
You might also be interested in the extended bibliographies on the topic 'Galaxy formation clusters' for particular source types:
Journal articles Dissertations / Theses
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