Relevant bibliographies by topics / Star cluster formation and evolution

Contents

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

Academic literature on the topic 'Star cluster formation and evolution'

Author: Grafiati
Published: 10 March 2023
Last updated: 19 July 2025

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Journal articles on the topic "Star cluster formation and evolution"

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Kroupa, Pavel. "Star-cluster formation and evolution." Proceedings of the International Astronomical Union 2, S237 (2006): 230–37. http://dx.doi.org/10.1017/s1743921307001524.

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AbstractStar clusters are observed to form in a highly compact state and with low star-formation efficiencies, and only 10 per cent of all clusters appear to survive to middle- and old-dynamical age. If the residual gas is expelled on a dynamical time the clusters disrupt. Massive clusters may then feed a hot kinematical stellar component into their host-galaxy's field population thereby thickening galactic disks, a process that theories of galaxy formation and evolution need to accommodate. If the gas-evacuation time-scale depends on cluster mass, then a power-law embedded-cluster mass functi
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Parmentier, Geneviève. "Early dynamical evolution of star cluster systems." Proceedings of the International Astronomical Union 5, S266 (2009): 87–94. http://dx.doi.org/10.1017/s1743921309990913.

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AbstractViolent relaxation, the protocluster dynamical response to the expulsion of its residual star-forming gas, is a short albeit crucial episode in the evolution of star clusters and star cluster systems. Because it is heavily driven by cluster-formation and environmental conditions, it is a potentially highly rewarding phase in terms of probing star formation and galaxy evolution. In this contribution, I review how cluster-formation and environmental conditions affect the shape of the young cluster mass function and the relation between the present star-formation rate of galaxies and the
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Vesperini, Enrico. "Star cluster dynamics." Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences 368, no. 1913 (2010): 829–49. http://dx.doi.org/10.1098/rsta.2009.0260.

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Dynamical evolution plays a key role in shaping the current properties of star clusters and star cluster systems. A detailed understanding of the effects of evolutionary processes is essential to be able to disentangle the properties that result from dynamical evolution from those imprinted at the time of cluster formation. In this review, I focus my attention on globular clusters, and review the main physical ingredients driving their early and long-term evolution, describe the possible evolutionary routes and show how cluster structure and stellar content are affected by dynamical evolution.
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Ishchenko, M., V. Masliukh, M. Hradov, P. Berczik, B. Shukirgaliyev, and C. Omarov. "Dynamical evolution of the open clusters with different star formation efficiencies and orbital parameters." Astronomy & Astrophysics 694 (January 30, 2025): A33. https://doi.org/10.1051/0004-6361/202452336.

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Context. Open star clusters are dynamic systems whose evolution is critically influenced by initial conditions such as star formation efficiency and orbital parameters. Understanding their dissolution mechanisms provides insight into stellar population dynamical mixing in the Milky Way. Aims. We aim to investigate the dynamical evolution and dissolution of initially non-virialised open clusters by examining how different global star formation efficiencies and orbital characteristics impact the cluster longevity and structural changes. We followed the evolution of the clusters up to their disso
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Zepf, Stephen E. "The Formation and Evolution of Star Clusters and Galaxies." Highlights of Astronomy 13 (2005): 347–49. http://dx.doi.org/10.1017/s1539299600015938.

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AbstractThis paper addresses the questions of what we have learned about how and when dense star clusters form, and what studies of star clusters have revealed about galaxy formation and evolution. One important observation is that globular clusters are observed to form in galaxy mergers and starbursts in the local universe, which both provides constraints on models of globular cluster formation, and suggests that similar physical conditions existed when most early-type galaxies and their globular clusters formed in the past. A second important observation is that globular cluster systems typi
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Gieles, Mark. "Star cluster disruption." Proceedings of the International Astronomical Union 5, S266 (2009): 69–80. http://dx.doi.org/10.1017/s1743921309990895.

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AbstractStar clusters are often used as tracers of major star-formation events in external galaxies as they can be studied out to much greater distances than individual stars. It is vital to understand their evolution if they are used to derive, for example, the star-formation history of their host galaxy. More specifically, we want to know how cluster lifetimes depend on their environment and on structural properties such as mass and radius. This review presents a theoretical overview of the early evolution of star clusters and the consequent long-term survival chances. It is suggested that c
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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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Clarke, C. J. "Star Formation in Large N Clusters." Symposium - International Astronomical Union 207 (2002): 489–98. http://dx.doi.org/10.1017/s0074180900224297.

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We focus here on the gas dynamics of cluster formation and the early stellar dynamical evolution of young clusters. We point out that the condition that a cloud can fragment into a large number of pieces places rather particular constraints on its initial state; we also review the processes that shape the stellar IMF in cluster formation simulations. We show how N-body calculations and observations can be combined to discover the properties of clusters at the point at which they first become stellar dynamical (as opposed to gas dynamical systems). Finally, we touch on the question of how proto
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Fensch, Jérémy, Pierre-Alain Duc, Médéric Boquien, et al. "Massive star cluster formation and evolution in tidal dwarf galaxies." Astronomy & Astrophysics 628 (August 2019): A60. http://dx.doi.org/10.1051/0004-6361/201834403.

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Context. The formation of globular clusters remains an open debate. Dwarf starburst galaxies are efficient at forming young massive clusters with similar masses as globular clusters and may hold the key to understanding their formation. Aims. We study star cluster formation in a tidal debris, including the vicinity of three tidal dwarf galaxies, in a massive gas-dominated collisional ring around NGC 5291. These dwarfs have physical parameters that differ significantly from local starbursting dwarfs. They are gas rich, highly turbulent, their gas metallicity is already enriched up to half solar
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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.

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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
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Dissertations / Theses on the topic "Star cluster formation and evolution"

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Adamo, A., J. E. Ryon, M. Messa, et al. "Legacy ExtraGalactic UV Survey with The Hubble Space Telescope: Stellar Cluster Catalogs and First Insights Into Cluster Formation and Evolution in NGC 628." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/624449.

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We report the large effort that is producing comprehensive high-level young star cluster (YSC) catalogs for a significant fraction of galaxies observed with the Legacy ExtraGalactic UV Survey (LEGUS) Hubble treasury program. We present the methodology developed to extract cluster positions, verify their genuine nature, produce multiband photometry (from NUV to NIR), and derive their physical properties via spectral energy distribution fitting analyses. We use the nearby spiral galaxy NGC 628 as a test case for demonstrating the impact that LEGUS will have on our understanding of the formation
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Messa, M., A. Adamo, G. Östlin, et al. "The young star cluster population of M51 with LEGUS – I. A comprehensive study of cluster formation and evolution." OXFORD UNIV PRESS, 2018. http://hdl.handle.net/10150/626277.

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Recently acquired WFC3 UV (F275W and F336W) imaging mosaics under the Legacy Extragalactic UV Survey (LEGUS), combined with archival ACS data of M51, are used to study the young star cluster (YSC) population of this interacting system. Our newly extracted source catalogue contains 2834 cluster candidates, morphologically classified to be compact and uniform in colour, for which ages, masses and extinction are derived. In this first work we study the main properties of the YSC population of the whole galaxy, considering a mass-limited sample. Both luminosity and mass functions follow a power-la
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Simanton, Lesley Ann. "Star Cluster Populations in the Spiral Galaxy M101." University of Toledo / OhioLINK, 2015. http://rave.ohiolink.edu/etdc/view?acc_num=toledo1437587267.

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Anders, Peter. "Formation and evolution of star clusters in interacting galaxies." Doctoral thesis, [S.l.] : [s.n.], 2006. http://webdoc.sub.gwdg.de/diss/2006/anders.

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Goodwin, S. P. "The early dynamical evolution of globular clusters." Thesis, University of Sussex, 1997. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.360496.

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Lyo, A.-Ran Physical Environmental &amp Mathematical Sciences Australian Defence Force Academy UNSW. "The nearby young [special character] Chamaeleontis cluster as a laboratory for star formation and evolution." Awarded by:University of New South Wales - Australian Defence Force Academy. School of Physical, Environmental and Mathematical Sciences, 2004. http://handle.unsw.edu.au/1959.4/38707.

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[Special characters cannot be displayed. Please see the pdf version of the Abstract for an accurate reproduction.] We studied the circumstellar discs, the initial mass function (IMF), mass distribution, binarity and the fundamental properties of the [special character] 9 Myr-old pre-main sequence (PMS) [special character] Chamaeleontis cluster. Using JHKL colour-colour and colour-excess diagrams, we found the circumstellar disc fraction to be [special character] 0.60 among the late-type members. Four stars with [special character] (K - L) > 0.4 were identified as experiencing ongoing accretio
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Dorval, Julien. "Multi-scale approach of the formation and evolution of star clusters." Thesis, Strasbourg, 2016. http://www.theses.fr/2016STRAE021/document.

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Les jeunes amas d'étoiles sont sous-structurés et évoluent dynamiquement pour former des amas sphériques à l'équilibre. Je présente une nouvelle méthode pour générer des conditions initiales réalistes pour simuler ce processus: la fragmentation de Hubble-Lemaitre. Je laisse le système développer spontanément des surdensités au cours d'une expansion du système. Le modèle résultant se compare bien aux simulations hydrodynamiques de formation stellaire et aux observations des jeunes amas. Le modèle fragmenté s'effondre de manière plus douce qu'un modèle uniforme. L'injection d'une population d'ét
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Rudnick, Gregory, Jacqueline Hodge, Fabian Walter, et al. "Deep CO(1–0) Observations of z = 1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies." IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/627107.

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We present an extremely deep CO(1-0) observation of a confirmed z = 1.62 galaxy cluster. We detect two spectroscopically confirmed cluster members in CO(1-0) with signal-to-noise ratio >5. Both galaxies have log (M-star/M-circle dot) > 11 and are gas rich, with M-mol/(M-star + M-mol) similar to 0.17-0.45. One of these galaxies lies on the star formation rate (SFR)-M-star sequence, while the other lies an order of magnitude below. We compare the cluster galaxies to other SFR-selected galaxies with CO measurements and find that they have CO luminosities consistent with expectations given their i
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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.

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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
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Ziosi, Brunetto Marco. "The impact of stellar evolution and dynamics on the formation of compact-object binaries." Doctoral thesis, Università degli studi di Padova, 2015. http://hdl.handle.net/11577/3424212.

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The aim of this work is to study the formation and evolution of double compact-object binaries (DCOBs, i.e. black hole-black hole, black hole-neutron star and neutron star-neutron star binaries) in young (< 100 Myr) dense (>~ 10^3 star/pc^3) star clusters (YSCs). DCOBs, when merging, are expected to be powerful sources of gravitational waves (GWs) observable by Virgo and LIGO detectors. Best merger candidates (BMCs), i.e. those sources with a chance to be observed, have a coalescence timescale shorter than one Hubble time (t_H) and produce a signal strong enough (strain >~ 10^-21) to be
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Books on the topic "Star cluster formation and evolution"

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Kenneth, Janes, and Astronomical Society of the Pacific. Summer Scientific Meeting, eds. The Formation and evolution of star clusters. Astronomical Society of the Pacific, 1991.

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San Roman, Izaskun. The Formation and Evolution of M33 as Revealed by Its Star Clusters. Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-7327-5.

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1968-, Alves João F., Elmegreen Bruce G, Girart Josep Miquel, and Trimble Virginia, eds. Computational star formation: Proceedings of the 270th Symposium of the International Astronomical Union held in Barcelona, Catalonia, Spain, May 31-June 4, 2010. Cambridge University Press, 2011.

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Lamers, Henny J. G. L. M., 1941-, Smith Linda J, and Nota Antonella, eds. The formation and evolution of massive young star clusters: Proceedings of a meeting held in Cancun, Mexico, 17-21 November 2003. Astronomical Society of the Pacific, 2004.

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Smith, Linda J., and L. B. F. M. Waters. Mass loss from stars and the evolution of stellar clusters: Proceedings of a workshop held at Lunteren, The Netherlands, 29 May-1 June 2006. Astronomical Society of the Pacific, 2008.

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Bodenheimer, Peter. Principles of star formation. Springer, 2011.

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Samuel, Angela E. The nature of star formation in the Trapezium Cluster. the Australian National University Library, 1993.

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Bo, Reipurth, and Astronomical Society of the Pacific., eds. Handbook of star forming regions. Astronomical Society of the Pacific, 2008.

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Hartmann, Lee. Accretion processes in star formation. 2nd ed. Cambridge University Press, 2009.

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Lada, Charles J., and Nikolaos D. Kylafis, eds. The Physics of Star Formation and Early Stellar Evolution. Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3642-6.

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Book chapters on the topic "Star cluster formation and evolution"

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Fritze, Uta, and V. Alvensleben. "Star and Globular Cluster Formation in Mergers." In New Light on Galaxy Evolution. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0229-9_88.

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Kodama, T., and R. G. Bower. "Global Star Formation History in Rich Cluster Cores." In The Evolution of Galaxies. Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-017-3313-7_156.

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Theis, Christian. "On a Formation Scenario of Star Clusters." In The Evolution of Galaxies. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-3311-3_11.

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De Marchi, Guido. "The Stellar Mass Function of Galactic Clusters and Its Evolution." In Open Issues in Local Star Formation. Springer Netherlands, 2003. http://dx.doi.org/10.1007/1-4020-2600-5_2.

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Palla, F. "Isolated and Clustered Star Formation: Observations and Theoretical Models." In Starbursts Triggers, Nature, and Evolution. Springer Berlin Heidelberg, 1998. http://dx.doi.org/10.1007/978-3-662-29742-1_4.

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Parmentier, Geneviève. "What cluster gas expulsion can tell us about star formation, cluster environment and galaxy evolution." In Reviews in Modern Astronomy. Wiley-VCH Verlag GmbH & Co. KGaA, 2010. http://dx.doi.org/10.1002/9783527629190.ch10.

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Li, Chengyuan. "The Formation and Evolution of Blue Straggler Stars in Globular Cluster." In Springer Theses. Springer Singapore, 2017. http://dx.doi.org/10.1007/978-981-10-5681-9_4.

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San Roman, Izaskun. "Erratum to: The Formation and Evolution of M33 as Revealed by Its Star Clusters." In Springer Theses. Springer New York, 2013. http://dx.doi.org/10.1007/978-1-4614-7327-5_7.

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Colpi, Monica, and Bernadetta Devecchi. "Dynamical Formation and Evolution of Neutron Star and Black Hole Binaries in Globular Clusters." In Physics of Relativistic Objects in Compact Binaries: From Birth to Coalescence. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9264-0_5.

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Fritze-v. Alvensleben, Uta. "Star Formation Efficiencies and Star Cluster Formation." In Starbursts. Springer Netherlands, 2005. http://dx.doi.org/10.1007/1-4020-3539-x_36.

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Conference papers on the topic "Star cluster formation and evolution"

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Mastrobuono-Battisti, Alessandra, and Hagai B. Perets. "The formation and evolution of nuclear star clusters." In Proceedings of the MG14 Meeting on General Relativity. WORLD SCIENTIFIC, 2017. http://dx.doi.org/10.1142/9789813226609_0295.

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Palouš, Jan, Richard Wünsch, Vasile Mioc, Cristiana Dumitrache, and Nedelia A. Popescu. "Star Formation and Evolution of Galaxies." In EXPLORING THE SOLAR SYSTEM AND THE UNIVERSE. AIP, 2008. http://dx.doi.org/10.1063/1.2993679.

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Smith, Randall K., Meg H. Abraham, Ryan Allured, et al. "Arcus: exploring the formation and evolution of clusters, galaxies, and stars." In UV, X-Ray, and Gamma-Ray Space Instrumentation for Astronomy XX, edited by Oswald H. Siegmund. SPIE, 2017. http://dx.doi.org/10.1117/12.2272818.

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Smith, Randall K., Marshall Bautz, Joel Bregman, et al. "Arcus: exploring the formation and evolution of clusters, galaxies, and stars." In Space Telescopes and Instrumentation 2022: Ultraviolet to Gamma Ray, edited by Jan-Willem A. den Herder, Kazuhiro Nakazawa, and Shouleh Nikzad. SPIE, 2022. http://dx.doi.org/10.1117/12.2628628.

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Charlton, Jane C., Robert Minchin, and Emmanuel Momjian. "Star Formation in Tidal Debris." In THE EVOLUTION OF GALAXIES THROUGH THE NEUTRAL HYDROGEN WINDOW. AIP, 2008. http://dx.doi.org/10.1063/1.2973574.

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Skillman, Evan D., Robert Minchin, and Emmanuel Momjian. "The HI∕Star Formation Connection." In THE EVOLUTION OF GALAXIES THROUGH THE NEUTRAL HYDROGEN WINDOW. AIP, 2008. http://dx.doi.org/10.1063/1.2973621.

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D'Antona, Francesca, Paolo Ventura, Roald Guandalini, Sara Palmerini, and Maurizio Busso. "Lithium, AGB and the Formation of Globular Clusters." In IXTH TORINO WORKSHOP ON EVOLUTION AND NUCLEOSYNTHESIS IN AGB STARS AND THE IIND PERUGIA WORKSHOP ON NUCLEAR ASTROPHYSICS. AIP, 2008. http://dx.doi.org/10.1063/1.2916988.

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Kobulnicky, Chip. "Star Formation At High Redshift." In THE EVOLUTION OF STARBURSTS: The 331st Wilhelm and Else Heraeus Seminar. AIP, 2005. http://dx.doi.org/10.1063/1.2035009.

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Donahue, Megan, Sebastian Heinz, and Eric Wilcots. "Signatures of Star Formation in Brightest Cluster Galaxies." In THE MONSTER’S FIERY BREATH: FEEDBACK IN GALAXIES, GROUPS, AND CLUSTERS. AIP, 2009. http://dx.doi.org/10.1063/1.3293027.

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Fuller, Gary, Jan Forbrich, Jill Rathborne, Steven Longmore, and Sergio Molinari. "Star and Stellar Cluster Formation: ALMA-SKA Synergies." In Advancing Astrophysics with the Square Kilometre Array. Sissa Medialab, 2015. http://dx.doi.org/10.22323/1.215.0152.

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Reports on the topic "Star cluster formation and evolution"

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Weaver, J. H. Cluster Formation and Evolution on Semiconductor Surface. Defense Technical Information Center, 1992. http://dx.doi.org/10.21236/ada259190.

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Hair. L52003 Application of the Crack Layer Theory for Understanding and Modeling of SCC in High Pressure. Pipeline Research Council International, Inc. (PRCI), 2003. http://dx.doi.org/10.55274/r0010893.

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A stochastic features of SCC colony, such as corrosion pit distribution, SC crack initiation from the pits and SC crack aspect ratio, SC crack cluster formation, SC cluster interaction and instability, are observed and characterized. A concept of a single crack equivalent to a cluster of cracks is introduced to simplify computational work on clusters evolution and instability. Various criteria of equivalence for different stages of clusters evolution are discussed. An accelerated test with a number of accelerating factors has been designed and performed for simulation of individual SC crack gr
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