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Journal articles on the topic 'Formation histories'

Author: Grafiati

Published: 31 May 2025

Last updated: 31 July 2025

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1

Tosi, Monica. "Star formation histories of resolved galaxies." Proceedings of the International Astronomical Union 4, S258 (2008): 61–72. http://dx.doi.org/10.1017/s1743921309031718.

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AbstractThe colour-magnitude diagrams of resolved stellar populations are the best tool to study the star formation histories of the host galactic regions. In this review the method to derive star formation histories by means of synthetic colour-magnitude diagrams is briefly outlined, and the results of its application to resolved galaxies of various morphological types are summarized. It is shown that all the galaxies studied so far were already forming stars at the lookback time reached by the observational data, independently of morphological type and metallicity. Early-type galaxies have f

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2

Cohn, J. D., and Martin White. "The formation histories of galaxy clusters." Astroparticle Physics 24, no. 4-5 (2005): 316–33. http://dx.doi.org/10.1016/j.astropartphys.2005.07.006.

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3

Chase, Michelle. "“A Cuba That Keeps Unsettling”." Radical History Review 2020, no. 136 (2020): 209–16. http://dx.doi.org/10.1215/01636545-7857380.

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Abstract Two young Cuban historians, Ailynn Torres Santana and Diosnara Ortega González, discuss their forthcoming book of oral histories with Cuban women. They describe their methodology, their intellectual formation, and the reception of gender studies and oral history in the Cuban academy.

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4

Butcher, H. R. "The star formation histories of the Magellanic Clouds." Symposium - International Astronomical Union 148 (1991): 138. http://dx.doi.org/10.1017/s007418090020020x.

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Existing observations of the Magellanic Clouds suggest substantially different star-forming histories for the two systems. The reliability of this conclusion is discussed in the context of the uncertainties and age resolutions of various empirical methods of studying galaxy evolution. An attempt is also made to relate likely evolutionary scenarios for the Clouds to the histories of other Local Group systems, to the evolution seen in galaxies at high redshift, and to possible histories determined by interaction with the Galaxy.

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5

Leach, Belinda. "A clash of histories." Focaal 2008, no. 51 (2008): 43–56. http://dx.doi.org/10.3167/fcl.2008.510105.

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This article considers the confrontations between immigrant and non-immigrant workers in the workplace and the implications of these confrontations for workplace unity and class formation. Contributing to scholarship at the intersection of history, class, and migration, the article argues that workers bring to work histories that are constructed as oppositional. The roots of these oppositions lie in shared but different histories of dispossession and migration, masked by dominant cultural and class narratives, which privilege non-immigrant histories that are class-based, masculinist, and natio

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Beniamini, Paz, Kenta Hotokezaka, Alexander van der Horst, and Chryssa Kouveliotou. "Formation rates and evolution histories of magnetars." Monthly Notices of the Royal Astronomical Society 487, no. 1 (2019): 1426–38. http://dx.doi.org/10.1093/mnras/stz1391.

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Buchalter, Ari, Raul Jimenez, and Marc Kamionkowski. "Galactosynthesis: halo histories, star formation and discs." Monthly Notices of the Royal Astronomical Society 322, no. 1 (2001): 43–66. http://dx.doi.org/10.1046/j.1365-8711.2001.04031.x.

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8

Brown, Thomas M. "Star formation histories in the Local Group." New Astronomy Reviews 49, no. 7-9 (2005): 474–77. http://dx.doi.org/10.1016/j.newar.2005.08.025.

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9

Hoyle, Ben, Rita Tojeiro, Raul Jimenez, Alan Heavens, Chris Clarkson, and Roy Maartens. "TESTING HOMOGENEITY WITH GALAXY STAR FORMATION HISTORIES." Astrophysical Journal 762, no. 1 (2012): L9. http://dx.doi.org/10.1088/2041-8205/762/1/l9.

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10

Ledinauskas, E., and K. Zubovas. "Reignited star formation in dwarf galaxies that were quenched during reionization." Astronomy & Astrophysics 615 (July 2018): A64. http://dx.doi.org/10.1051/0004-6361/201832824.

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Context. Irregular dwarf galaxies of the Local Group have very varied properties and star formation histories. Some of them formed the majority of their stars very late compared to others. Extreme examples of this are Leo A and Aquarius, which reached the peak of star formation at z < 1 (more than 6 Gyr after the Big Bang). This fact seemingly challenges the ΛCDM cosmological framework because the dark matter halos of these galaxies on average should assemble the majority of their masses before z ~ 2 (<3 Gyr after the Big Bang). Aims. We investigate whether the delayed star formation his

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11

de la Rosa, Ignacio G., Robert N. Proctor, Claudia Mendes de Oliveira, Duncan A. Forbes, Roberto Cid Fernandes, and Abilio Mateus. "The star formation histories of fossil group galaxies." Proceedings of the International Astronomical Union 5, S262 (2009): 321–22. http://dx.doi.org/10.1017/s1743921310003042.

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AbstractA comparison is carried out among the star formation histories of early-type galaxies in fossil groups, clusters and low density environments. Although they show similar evolutionary histories, a significant fraction of the fossils are younger than their counterparts, suggesting that they can be precursors of the isolated ETG galaxies.

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12

Baycroft, Timothy. "Histories of Nations and Borders: Critical Reflections." Do historians fail in listening to each other? Methodological Challenges for Historical Dialogue 1, no. 1 (2022): 92–107. http://dx.doi.org/10.54881/111nbtb.

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Examining the question of ‘which history’ of a nation emerges over time and why, this article interrogates the ways in which histories and borders come to acquire symbolic significance and become ‘national histories’ and ‘national borders’. It begins with a thorough analysis of the elements that contribute to and the forces which have an impact upon the development of national identity, national symbolism, and national memory. Then, drawing from a range of examples, it provides serious critical reflection on the work of historians and the nature of the questions that need to be asked in order

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13

Wyse, Rosemary F. G. "The star-formation history of the Milky Way Galaxy." Proceedings of the International Astronomical Union 4, S258 (2008): 11–22. http://dx.doi.org/10.1017/s1743921309031664.

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AbstractThe star-formation histories of the main stellar components of the Milky Way constrain critical aspects of galaxy formation and evolution. I discuss recent determinations of such histories, together with their interpretation in terms of theories of disk galaxy evolution.

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14

Porat, Dan A. "One Historian, Two Histories: Jacob Katz and the Formation of a National Israeli Identity." Jewish Social Studies: History, Culture, and Society 9, no. 3 (2003): 56–75. http://dx.doi.org/10.2979/jss.2003.9.3.56.

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Porat, Dan A. "One Historian, Two Histories: Jacob Katz and the Formation of a National Israeli Identity." Jewish Social Studies 9, no. 3 (2003): 56–75. http://dx.doi.org/10.1353/jss.2003.0023.

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16

Feathers, Colton R., Mihir Kulkarni, and Eli Visbal. "From dark matter minihalos to large-scale radiative feedback: a self-consistent 3D simulation of the first stars and galaxies using neural networks." Journal of Cosmology and Astroparticle Physics 2025, no. 02 (2025): 043. https://doi.org/10.1088/1475-7516/2025/02/043.

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Abstract A key obstacle to accurate models of the first stars and galaxies is the vast range of distance scales that must be considered. While star formation occurs on sub-parsec scales within dark matter (DM) minihalos, it is influenced by large-scale baryon-dark matter streaming velocities (v bc) and Lyman-Werner (LW) radiative feedback which vary significantly on scales of ∼100 Mpc. We present a novel approach to this issue in which we utilize artificial neural networks (NNs) to emulate the Population III (PopIII) and Population II (PopII) star formation histories of many small-scale cells

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17

Aloisi, Alessandra. "Star-Formation Histories of Resolved Galaxies in the Local Volume." Proceedings of the International Astronomical Union 12, S316 (2015): 61–69. http://dx.doi.org/10.1017/s1743921315010583.

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AbstractColor-magnitude diagrams of resolved stellar populations are the most powerful tool to derive the star formation histories of galaxies. In this review the method to infer star formation histories by comparing synthetic color-magnitude diagrams to deep, high-precision, multi-color photometry is briefly outlined, and our current knowledge of the star formation history of systems within the local Volume is summarized.

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18

Nasr-El-Din, Hisham A. "Formation Damage Induced by Chemical Treatments: Case Histories." Journal of Energy Resources Technology 127, no. 3 (2005): 214–24. http://dx.doi.org/10.1115/1.1924464.

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This study discusses formation damage mechanisms that were caused by commonly used chemical treatments. The chemicals used in these treatments included a scale inhibitor, a biocide-corrosion inhibitor, an in situ gelled acid, a full-strength mud acid, and a mutual solvent. These treatments were designed to remove a known form of formation damage. However, they created new forms of formation damage, which resulted in a significant decline in the performance of the treated wells. Case histories that illustrate the initial and new formation damage mechanisms are explained in detail. Laboratory an

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19

Grebel, E. K. "Star Formation Histories of Local Group Dwarf Galaxies." Highlights of Astronomy 11, no. 1 (1998): 125–26. http://dx.doi.org/10.1017/s1539299600020190.

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The Local Group contains 37 currently known or probable member galaxies within a radius of 1.8 Mpc (Grebel 1997a). 31 of these galaxies are dwarf galaxies with MB > -17 mag. The most frequent galaxy types are low-mass, gas-poor dwarf spheroidal (dSph) galaxies, which are dominated by old and intermediate-age populations, and more massive, gas-rich dwarf irregular (dIrr) galaxies with recent star formation. DSph galaxies have been found mostly in close vicinity to the large spiral galaxies in the Local Group, while dirr galaxies tend to be more distant and isolated.

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20

Proctor, R. N., A. E. Sansom, and I. N. Reid. "Constraining the star formation histories of spiral bulges." Monthly Notices of the Royal Astronomical Society 311, no. 1 (2000): 37–49. http://dx.doi.org/10.1046/j.1365-8711.2000.03018.x.

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21

Dale, Daniel A., Gillian D. Beltz-Mohrmann, Arika A. Egan, et al. "RADIAL STAR FORMATION HISTORIES IN 15 NEARBY GALAXIES." Astronomical Journal 151, no. 1 (2015): 4. http://dx.doi.org/10.3847/0004-6256/151/1/4.

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22

Gilda, Sankalp, Antoine de Mathelin, Sabine Bellstedt, and Guillaume Richard. "Unsupervised Domain Adaptation for Constraining Star Formation Histories." Astronomy 3, no. 3 (2024): 189–207. http://dx.doi.org/10.3390/astronomy3030012.

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In astronomy, understanding the evolutionary trajectories of galaxies necessitates a robust analysis of their star formation histories (SFHs), a task complicated by our inability to observe these vast celestial entities throughout their billion-year lifespans. This study pioneers the application of the Kullback–Leibler Importance Estimation Procedure (KLIEP), an unsupervised domain adaptation technique, to address this challenge. By adeptly applying KLIEP, we harness the power of machine learning to innovatively predict SFHs, utilizing simulated galaxy models to forge a novel linkage between s

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23

Pereira-Santaella, Miguel, Almudena Alonso-Herrero, Luis Colina, et al. "Star-formation histories of local luminous infrared galaxies." Astronomy & Astrophysics 577 (May 2015): A78. http://dx.doi.org/10.1051/0004-6361/201425359.

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24

Arimoto, N. "Modeling of star formation histories of dwarf ellipticals." Proceedings of the International Astronomical Union 1, no. C198 (2005): 17–24. http://dx.doi.org/10.1017/s1743921305003418.

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25

Wyse, Rosemary F. G. "Star-formation histories, metallicity distributions and luminosity functions." Proceedings of the International Astronomical Union 5, H15 (2009): 180–81. http://dx.doi.org/10.1017/s1743921310008616.

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26

Skillman, Evan D. "Star formation histories in local group dwarf galaxies." New Astronomy Reviews 49, no. 7-9 (2005): 453–60. http://dx.doi.org/10.1016/j.newar.2005.08.022.

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27

Grebel, Eva K., Tsafrir Kolatt, and Wolfgang Brandner. "Orbits versus Star Formation Histories: A Progress Report." Symposium - International Astronomical Union 192 (1999): 447–50. http://dx.doi.org/10.1017/s0074180900204488.

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Milky Way dwarf companions and satellites of distant spirals seem to show a preference for polar orbits. We suggest that five out of six M31 dwarf spheroidal companions as well as two dwarf irregulars may also be located near a polar plane.We briefly discuss preliminary results from a statistical approach to study correlations between star formation histories and orbits of Local Group dwarf galaxies, such as a possible correlation between star formation episodes and galaxy separations.

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28

Dale, Daniel A., Kristin R. Anderson, Louis M. Bran, et al. "Radial Star Formation Histories in 32 Nearby Galaxies." Astronomical Journal 159, no. 5 (2020): 195. http://dx.doi.org/10.3847/1538-3881/ab7eb2.

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29

Aumer, Michael, Simon D. M. White, and Thorsten Naab. "The diverse formation histories of simulated disc galaxies." Monthly Notices of the Royal Astronomical Society 441, no. 4 (2014): 3679–95. http://dx.doi.org/10.1093/mnras/stu818.

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30

González Delgado, R. M., E. Pérez, R. Cid Fernandes, et al. "Spatially-resolved star formation histories of CALIFA galaxies." Astronomy & Astrophysics 607 (November 2017): A128. http://dx.doi.org/10.1051/0004-6361/201730883.

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This paper presents the spatially resolved star formation history (SFH) of nearby galaxies with the aim of furthering our understanding of the different processes involved in the formation and evolution of galaxies. To this end, we apply the fossil record method of stellar population synthesis to a rich and diverse data set of 436 galaxies observed with integral field spectroscopy in the CALIFA survey. The sample covers a wide range of Hubble types, with stellar masses ranging from M⋆ ~ 109 to 7 × 1011 M⊙. Spectral synthesis techniques are applied to the datacubes to retrieve the spatially res

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31

Maltempi, Anne. "Writing History in Renaissance Sicily: The Formation of Sicilian National Identity in the Work of Tommaso Fazello." Mediterranean Studies 29, no. 1 (2021): 4–31. http://dx.doi.org/10.5325/mediterraneanstu.29.1.4.

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Abstract This study illuminates the process of writing history in Renaissance Sicily. While Italian historians have offered revisionist histories of Sicily in the Medieval period, the same cannot be said for the Sicilian Renaissance. The existing gap in our understanding of Renaissance historiography with regard to Sicily is the result of a much more expansive tradition that can be traced from Dante and Petrarch to later Italian national histories such as those of Francesco DeSanctis and Benedetto Croce, not to mention Jacob Burckhardt. Anglophone historiography of the Renaissance also reflect

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32

Kutulukov, S. P. "FEATURES OF THE FORMATION OF THE NOMADIC UZBEK STATE IN THE CONTEXT OF CONSTRUCTIVISM." History of the Homeland 96, no. 4 (2021): 56–64. http://dx.doi.org/10.51943/1814-6961_2021_4_56.

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The peculiarities of the formation of medieval Turkic states are of particular interest dueto the political conditionality of the issue for the region. The revision of national histories gives rise to a lot of distortions, inaccuracies and manipulations both among professional historians and specialists in other fields. A constructivist approach in exploring and determining the main features of the formation of nomadic states in Central Asia is a prerequisite for further effective research of the idea of the Turkic Renaissance. The article attempts to constructivist understanding of the format

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33

Bell, E. F., R. G. Bower, R. S. de Jong, et al. "The star formation histories of Low Surface Brightness galaxies." International Astronomical Union Colloquium 171 (1999): 245–52. http://dx.doi.org/10.1017/s0252921100054403.

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AbstractNear-infrared images of a sample of red, blue and giant low surface brightness disk galaxies (LSBGs) were combined with optical data with the aim of constraining their star formation histories. Most LSBGs have strong colour gradients consistent with mean stellar age gradients. We find that LSBGs have a large range of ages and metallicities, spanning those observed in normal disk galaxies. In particular, red and blue LSBGs have very different star formation histories and represent two independent routes to low B band surface brightness. Blue LSBGs are well described by models with low,

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34

Meyer, Franz Michael. "Case Histories of Orogenic Gold Deposits." Minerals 13, no. 3 (2023): 369. http://dx.doi.org/10.3390/min13030369.

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This review compares genetic parameters of 12 orogenic gold deposits. The set of examples is considered to represent largely the variability of orogenic gold deposit (OGD) characteristics. The data are presented in tables and include following definitive parameters: regional geologic settings, nature of hosts rocks and mineralization, ore controlling structures, ages of host rocks and mineralization and timing of mineralization relative to metamorphism, hydrothermal alteration mineralogy and ore mineral assemblages, isotopic signatures, physical conditions of ore formation and proposed origin

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35

Pacifici, Camilla, Susan A. Kassin, Benjamin J. Weiner, et al. "THE EVOLUTION OF STAR FORMATION HISTORIES OF QUIESCENT GALAXIES." Astrophysical Journal 832, no. 1 (2016): 79. http://dx.doi.org/10.3847/0004-637x/832/1/79.

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36

Ricotti, Massimo, and Nickolay Y. Gnedin. "Formation Histories of Dwarf Galaxies in the Local Group." Astrophysical Journal 629, no. 1 (2005): 259–67. http://dx.doi.org/10.1086/431415.

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37

Hamedani Golshan, R., A. Javadi, and J. Th van Loon. "Star formation histories in NGC 147 and NGC 185." Journal of Physics: Conference Series 869 (June 2017): 012087. http://dx.doi.org/10.1088/1742-6596/869/1/012087.

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38

Plauchu-Frayn, I., A. Del Olmo, R. Coziol, and J. P. Torres-Papaqui. "The star formation histories of Hickson compact group galaxies." Astronomy & Astrophysics 546 (October 2012): A48. http://dx.doi.org/10.1051/0004-6361/201219916.

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39

Small, Emma E., David Bersier, and Maurizio Salaris. "Star formation histories of resolved galaxies – I. The method." Monthly Notices of the Royal Astronomical Society 428, no. 1 (2012): 763–77. http://dx.doi.org/10.1093/mnras/sts077.

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40

Bell, E. F., D. Barnaby, R. G. Bower, et al. "The star formation histories of low surface brightness galaxies." Monthly Notices of the Royal Astronomical Society 312, no. 3 (2000): 470–96. http://dx.doi.org/10.1046/j.1365-8711.2000.03180.x.

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41

Dolphin, A. E. "The star formation histories of two northern LMC fields." Monthly Notices of the Royal Astronomical Society 313, no. 2 (2000): 281–90. http://dx.doi.org/10.1046/j.1365-8711.2000.03197.x.

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42

Knebe, Alexander, Julien E. G. Devriendt, Asim Mahmood, and Joseph Silk. "Merger histories in warm dark matter structure formation scenarios." Monthly Notices of the Royal Astronomical Society 329, no. 4 (2002): 813–28. http://dx.doi.org/10.1046/j.1365-8711.2002.05017.x.

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43

Demarco, R., R. Gobat, P. Rosati, et al. "STAR FORMATION HISTORIES IN A CLUSTER ENVIRONMENT ATz∼ 0.84." Astrophysical Journal 725, no. 1 (2010): 1252–76. http://dx.doi.org/10.1088/0004-637x/725/1/1252.

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44

Dye, Simon. "Star formation histories from multiband photometry: a new approach." Monthly Notices of the Royal Astronomical Society 389, no. 3 (2008): 1293–305. http://dx.doi.org/10.1111/j.1365-2966.2008.13639.x.

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45

Zhang, Hong-Xin, Yu Gao, and Xu Kong. "Star formation histories within the Antennae galaxies (Arp 244)." Monthly Notices of the Royal Astronomical Society 401, no. 3 (2010): 1839–49. http://dx.doi.org/10.1111/j.1365-2966.2009.15759.x.

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46

Molinari, Sergio. "Star Formation Histories from Pan-Chromatic Infrared Continuum Surveys." Proceedings of the International Astronomical Union 5, H15 (2009): 802. http://dx.doi.org/10.1017/s1743921310011804.

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AbstractOne of the currently most disputed issues in Star Formation is the timeline of the whole process. Is it a “slow” process of cloud assembly which, mediated by magnetic fields, evolve toward turbulence-supported clumps which are eventually super-critical to collapse, e.g. McKee & Tan (2003)? Or do clumps originate in already super-critical state in the post-shock regions of large-scale Galactic converging flows, e.g. Hartmann et al. (2001) with a rapid collapse in a crossing time or so (Elmegreen 2000)?A pan-chromatic 1μm-1mm continuum view of cluster forming regions in their early s

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47

Poggianti, Bianca M., Ian Smail, Alan Dressler, et al. "The Star Formation Histories of Galaxies in Distant Clusters." Astrophysical Journal 518, no. 2 (1999): 576–93. http://dx.doi.org/10.1086/307322.

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48

Dye, Simon, Steve Eales, Lorenzo Moncelsi, and Enzo Pascale. "Evolution of the star formation histories of BLAST galaxies." Monthly Notices of the Royal Astronomical Society: Letters 407, no. 1 (2010): L69—L73. http://dx.doi.org/10.1111/j.1745-3933.2010.00907.x.

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49

Koleva, M., A. J. Cenarro, I. de la Rosa, P. Sanchez-Blazquez, and A. Vazdekis. "Star Formation Histories from Spectra: What Can We Believe?" EAS Publications Series 48 (2011): 87–89. http://dx.doi.org/10.1051/eas/1148021.

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50

Mathis, H., S. Charlot, and J. Brinchmann. "Extracting star formation histories from medium-resolution galaxy spectra." Monthly Notices of the Royal Astronomical Society 365, no. 2 (2006): 385–400. http://dx.doi.org/10.1111/j.1365-2966.2005.09790.x.

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