Relevant bibliographies by topics / Bar formation, galaxy evolution

Contents

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

Academic literature on the topic 'Bar formation, galaxy evolution'

Author: Grafiati
Published: 9 March 2023
Last updated: 31 July 2025

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Journal articles on the topic "Bar formation, galaxy evolution"

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Combes, Francoise. "Galaxy Dynamics: Secular Evolution and Accretion." Proceedings of the International Astronomical Union 6, S271 (2010): 119–26. http://dx.doi.org/10.1017/s1743921311017522.

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AbstractRecent results are reviewed on galaxy dynamics, bar evolution, destruction and re-formation, cold gas accretion, gas radial flows and AGN fueling, minor mergers. Some problems of galaxy evolution are discussed in particular, exchange of angular momentum, radial migration through resonant scattering, and consequences on abundance gradients, the frequency of bulgeless galaxies, and the relative role of secular evolution and hierarchical formation.
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Łokas, Ewa L. "An interesting case of the formation and evolution of a barred galaxy in the cosmological context." Astronomy & Astrophysics 642 (October 2020): L12. http://dx.doi.org/10.1051/0004-6361/202039425.

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Elongated, bar-like galaxies without a significant disk component, with little rotation support and no gas, often form as a result of tidal interactions with a galaxy cluster, as was recently demonstrated using the IllustrisTNG-100 simulation. Galaxies that exhibit similar properties are, however, also found to be infalling into the cluster for the first time. We use the same simulation to study in detail the history of such a galaxy over cosmic time in order to determine its origin. The bar appears to be triggered at t = 6.8 Gyr by the combined effect of the last significant merger with a sub
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Combes, Françoise. "Ring and Lens Formation." International Astronomical Union Colloquium 157 (1996): 286–98. http://dx.doi.org/10.1017/s0252921100049927.

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AbstractThe dynamical mechanism to form rings at Lindblad resonances in a barred galaxy is now well-known: due to its dissipative character, the gas is forced in a spiral structure, and experiences torques from the bar potential. Angular momentum is transferred until gas accumulates in the resonant rings. Some problems remain however to account for all observations, such as the very different time-scales for nuclear, inner and outer ring formation, while the three are frequently observed in the same galaxy; the shapes, orientations and thickness of the rings, etc... The adequacy of the present
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Athanassoula, E. "Evolution of Bars in Isolated and in Interacting Disk Galaxies." International Astronomical Union Colloquium 157 (1996): 309–20. http://dx.doi.org/10.1017/s0252921100049940.

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AbstractI use N-body simulations to follow the evolution of bars in both isolated and interacting disk galaxies. The pattern speeds of bars evolving in isolated galaxies decline gradually with time, due to transfer of angular momentum from the bar to other components in the galaxy. Both the form and amount of this decline depend on the model used. The fate of a bar in an interacting disk galaxy depends on the mass, central concentration and orbit of the perturber. The pattern speed, form and amplitude of the bar may change, the bar can become off-centered, or, more drastically, it can disappea
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Géron, Tobias, R. J. Smethurst, Chris Lintott, et al. "The Effects of Bar Strength and Kinematics on Galaxy Evolution: Slow Strong Bars Affect Their Hosts the Most." Astrophysical Journal 973, no. 2 (2024): 129. http://dx.doi.org/10.3847/1538-4357/ad66b7.

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Abstract We study how bar strength and bar kinematics affect star formation in different regions of the bar by creating radial profiles of EW[Hα] and Dn4000 using data from Sloan Digital Sky Survey-IV Mapping Nearby Galaxies at Apache Point Observatory (MaNGA). Bars in galaxies are classified as strong or weak using Galaxy Zoo DESI, and they are classified as fast and slow bars using the Tremaine–Weinberg method on stellar kinematic data from the MaNGA survey. In agreement with previous studies, we find that strong bars in star-forming (SF) galaxies have enhanced star formation in their center
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Neumann, Justus, Francesca Fragkoudi, Isabel Pérez, et al. "Stellar populations across galaxy bars in the MUSE TIMER project." Astronomy & Astrophysics 637 (May 2020): A56. http://dx.doi.org/10.1051/0004-6361/202037604.

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Stellar populations in barred galaxies save an imprint of the influence of the bar on the host galaxy’s evolution. We present a detailed analysis of star formation histories (SFHs) and chemical enrichment of stellar populations in nine nearby barred galaxies from the TIMER project. We used integral field observations with the MUSE instrument to derive unprecedented spatially resolved maps of stellar ages, metallicities, [Mg/Fe] abundances, and SFHs, as well as Hα as a tracer of ongoing star formation. We find a characteristic V-shaped signature in the SFH that is perpendicular to the bar major
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Géron, Tobias, R. J. Smethurst, Hugh Dickinson, et al. "Galaxy Zoo CEERS: Bar Fractions Up to z ∼ 4.0." Astrophysical Journal 987, no. 1 (2025): 74. https://doi.org/10.3847/1538-4357/add7d0.

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Abstract We study the evolution of the bar fraction in disk galaxies between 0.5 < z < 4.0 using multiband colored images from JWST Cosmic Evolution Early Release Science Survey (CEERS). These images were classified by citizen scientists in a new phase of the Galaxy Zoo (GZ) project called GZ CEERS. Citizen scientists were asked whether a strong or weak bar was visible in the host galaxy. After considering multiple corrections for observational biases, we find that the bar fraction decreases with redshift in our volume-limited sample (n = 398); from 2 5 − 4 + 6 % at 0.5 < z < 1.0 t
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López Gómez, Alejandro, Ruslan Gabbasov, and Isaura Luisa Fuentes-Carrera. "Numerical Study of Bar Suppression in Galaxy Models Due to Disc Heating." Galaxies 13, no. 2 (2025): 45. https://doi.org/10.3390/galaxies13020045.

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The process of bar formation, evolution and destruction is still a controversial topic regarding galaxy dynamics. Numerical simulations show that these phenomena strongly depend on physical and numerical parameters. In this work, we study the combined influence of the softening parameter, ϵ and disc mass fraction, md, on the formation and evolution of bars in isolated disc-halo models via N-body simulations with different particle resolutions. Previous studies indicate that the bar strength depends on md as ∝md−1, which is seen as a delay in bar formation. However, the distorsion parameter, η,
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Fraser-McKelvie, Amelia, Alfonso Aragón-Salamanca, Michael Merrifield, et al. "SDSS-IV MaNGA: spatially resolved star formation in barred galaxies." Monthly Notices of the Royal Astronomical Society 495, no. 4 (2020): 4158–69. http://dx.doi.org/10.1093/mnras/staa1416.

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ABSTRACT Bars inhabit the majority of local-Universe disc galaxies and may be important drivers of galaxy evolution through the redistribution of gas and angular momentum within discs. We investigate the star formation and gas properties of bars in galaxies spanning a wide range of masses, environments, and star formation rates using the Mapping Nearby Galaxies at APO galaxy survey. Using a robustly defined sample of 684 barred galaxies, we find that fractional (or scaled) bar length correlates with the host’s offset from the star formation main sequence. Considering the morphology of the Hα e
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Kataria, Sandeep Kumar, and Juntai Shen. "Importance of Initial Condition on Bar Secular Evolution: Role of Halo Angular Momentum Distribution Discontinuity." Astrophysical Journal 970, no. 1 (2024): 45. http://dx.doi.org/10.3847/1538-4357/ad5b58.

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Abstract The dark matter halo properties, for example, mass, spin, and concentration, play a significant role in the formation and evolution of bars in disk galaxies. This study highlights the importance of a new parameter: the dark matter halo angular momentum distribution in the disk’s central region. We experiment with N-body galaxy models having a disk and dark matter similar to Milky Way–type galaxies. In these models, we vary the discontinuity of the angular momentum distribution of the halo (the total spin is the same for all models). Our N-body experiments suggest that bar forms in all
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Dissertations / Theses on the topic "Bar formation, galaxy evolution"

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FANALI, ROSSELLA. "Bar-formation as driver of gas inflows in isolated disc galaxies." Doctoral thesis, Università degli Studi di Milano-Bicocca, 2015. http://hdl.handle.net/10281/96384.

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Stellar bars are a common feature in massive disc galaxies. On a theoretical ground, the response of gas to a bar is generally thought to cause nuclear starbursts and, possibly, AGN activity once the perturbed gas reaches the central super-massive black hole. By means of high resolution numerical simulations we detail the purely dynamical effects that a forming bar exerts on the gas of an isolated disc galaxy. The galaxy is initially unstable to the formation of non-axisymmetric structures, and within 1 Gyr it develops spiral arms that eventually evolve into a central stellar bar on kpc scale.
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Kraljic, Katarina. "Links between galaxy evolution, morphology and internal physical processes." Thesis, Paris 11, 2014. http://www.theses.fr/2014PA112286/document.

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Cette thèse a pour but de faire le lien entre l’évolution des galaxies, leur morphologie et les processus physiques internes, notamment la formation stellaire comme le résultat du milieu interstellaire turbulent et multiphase, en utilisant les simulations cosmologiques zoom-in, les simulations des galaxies isolées et en interaction, et le modèle analytique de la formation stellaire. Dans le chapitre 1, j’explique la motivation pour cette thèse et je passe brièvement en revue le contexte nécessaire lié à la formation des galaxies et la modélisation en utilisant les simulations numériques. Tout
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Williams, Michael J. "Early-type disk galaxies." Thesis, University of Oxford, 2011. http://ora.ox.ac.uk/objects/uuid:936168ab-f49a-410a-9e1b-80c7ad7cf556.

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In this thesis I investigate the dynamics and stellar populations of a sample of 28 edge-on early-type (S0--Sb) disk galaxies, 22 of which host a boxy or peanut-shaped bulge. I begin by constructing mass models of the galaxies based on their observed photometry and stellar kinematics. Subject to cosmologically motivated assumptions about the shape of dark haloes, I measure in a purely dynamical way their stellar and dark masses. I make a preliminary comparison between the dynamically determined stellar masses and those predicted by stellar population models. I then compare the Tully-Fisher (lu
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Croton, Darren. "Galaxy Formation and Evolution." Diss., lmu, 2005. http://nbn-resolving.de/urn:nbn:de:bvb:19-44059.

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Thomas, Daniel. "Chemical evolution and galaxy formation." Diss., lmu, 2000. http://nbn-resolving.de/urn:nbn:de:bvb:19-4637.

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Romano, Donatella. "Chemical evolution and galaxy formation." Doctoral thesis, SISSA, 2002. http://hdl.handle.net/20.500.11767/4041.

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Following a review of the basic ingredients necessary for constructing models of galactic chemical evolution, with a special emphasis on the issue of stellar evolution and nucleosynthesis (which is treated in detail in Chapter 2), I continue with the basic equations that one needs to solve in order to follow the chemical evolution of a system of gas and stars in time and space. The assumptions of the models I have handled with the aim of addressing different aspects of the formation and evolution of the Milky Way and elliptical galaxies are discussed in Chapter 3. In Chapters 4 and 5,
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Linke, Laila Maria [Verfasser]. "Testing models of galaxy formation and evolution with galaxy-galaxy-galaxy lensing / Laila Maria Linke." Bonn : Universitäts- und Landesbibliothek Bonn, 2021. http://d-nb.info/1235524469/34.

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Burton, Christopher Steven. "The environmental dependence of galaxy evolution." Thesis, University of Hertfordshire, 2013. http://hdl.handle.net/2299/12572.

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Observations of galaxy environments have revealed numerous correlations associated with their intrinsic properties. It is therefore clear that if we are to understand the processes by which galaxies form and evolve, we have to consider the role of their immediate environment and how these trends change across cosmic time. In this thesis, I investigate the relationship between the environmental densities of galaxies and their associated properties by developing and implementing a novel approach to measuring galaxy environments on individual galaxy scales with Voronoi tessellations. Using optica
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Moustakas, John. "Spectral Diagnostics of Galaxy Evolution." Diss., The University of Arizona, 2006. http://hdl.handle.net/10150/305142.

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Despite considerable progress in recent years, a complete description of the physical drivers of galaxy formation and evolution remains elusive, in part because of our poor understanding of star formation, and how star formation in galaxies is regulated by feedback from supernovae and massive stellar winds. Insight into the star formation histories of galaxies, and the interplay between star formation and feedback, can be gained by measuring their chemical abundances, which until recently has only been possible for galaxies in the nearby universe. However, reliable star formation and abundance
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Bothwell, Matthew Stuart. "Galaxy evolution : near and far." Thesis, University of Cambridge, 2011. https://www.repository.cam.ac.uk/handle/1810/265602.

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The formation of stars from interstellar gas is the cornerstone of galaxy evolution. This thesis represents work undertaken in order to characterise the role of cool interstellar gas, and its relation to star formation, in galaxy evolution across cosmic time. In particular, it concentrates on star forming galaxies at the extremes of the galaxy assembly spectrum - extremely faint dwarfs, and extremely luminous starbursts - in an attempt to test the limits of galaxy evolution models. The thesis falls into two complimentary halves, addressing topics in the low redshift and high redshift Universe
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Books on the topic "Bar formation, galaxy evolution"

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Van den Bosch, Frank, 1969- and White S, eds. Galaxy formation and evolution. Cambridge University Press, 2010.

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Spinrad, Hyron. Galaxy formation and evolution. Springer, 2005.

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Källander, Daniel. Computational galaxy formation. Acta Universitatis Upsaliensis, 1996.

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Renzini, Alvio, and Ralf Bender, eds. Multiwavelength Mapping of Galaxy Formation and Evolution. Springer Berlin Heidelberg, 2005. http://dx.doi.org/10.1007/b96746.

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Ferreras, Ignacio. Fundamentals of Galaxy Dynamics, Formation and Evolution. UCL Press, 2019.

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Papaderos, Polychronis, Simone Recchi, and Gerhard Hensler, eds. Dwarf Galaxies: Keys to Galaxy Formation and Evolution. Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-22018-0.

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Boer, Klaas S. de. GAIA: Composition, formation, and evolution of the galaxy. ESA Publications, 2000.

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Gnedin, Nickolay Y., Simon C. O. Glover, Ralf S. Klessen, and Volker Springel. Star Formation in Galaxy Evolution: Connecting Numerical Models to Reality. Edited by Yves Revaz, Pascale Jablonka, Romain Teyssier, and Lucio Mayer. Springer Berlin Heidelberg, 2016. http://dx.doi.org/10.1007/978-3-662-47890-5.

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Bland-Hawthorn, J. The origin of the galaxy and local group: Saas-Fee Advanced Course 37. Springer, 2014.

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Taiwan) Galaxy Mergers in An Evolving Universe (Conference) (2011 Hua-lien shih. Galaxy mergers in an evolving universe: Proceedings of a conference held at Farglory Hotel, Hualien, Taiwan, 23-28 October 2011. Astronomical Society of the Pacific, 2013.

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Book chapters on the topic "Bar formation, galaxy evolution"

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Norman, C. A., H. Hasan, and J. A. Sellwood. "Bar dissolution and bulge formation." In New Light on Galaxy Evolution. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0229-9_138.

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Noguchi, Masafumi. "Bar Formation by Galaxy-Galaxy Interactions." In Astrophysics and Space Science Library. Springer Netherlands, 2004. http://dx.doi.org/10.1007/978-1-4020-2862-5_20.

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Bergeron, J. "Galaxy Formation and Evolution." In Astrophysics and Space Science Proceedings. Springer Netherlands, 2009. http://dx.doi.org/10.1007/978-1-4020-9190-2_25.

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Nagamine, Kentaro, Naveen Reddy, Emanuele Daddi, and Mark T. Sargent. "Galaxy Formation and Evolution." In Gamma-Ray Bursts. Springer Netherlands, 2016. http://dx.doi.org/10.1007/978-94-024-1279-6_4.

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Braine, Jonathan, P. A. Duc, U. Lisenfeld, et al. "On-Going Galaxy Formation." In The Evolution of Galaxies. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-3311-3_92.

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Möllenhoff, C., M. Matthias, and O. E. Gerhard. "The Central Bar in M 94." In New Light on Galaxy Evolution. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0229-9_134.

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Silk, J. "From Star To Galaxy Formation." In Starbursts Triggers, Nature, and Evolution. Springer Berlin Heidelberg, 1998. http://dx.doi.org/10.1007/978-3-662-29742-1_7.

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Chiba, M., and B. B. Nath. "Photoionization Effects on Galaxy Formation." In New Light on Galaxy Evolution. Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0229-9_64.

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Silk, Joseph. "Towards a Theory of Galaxy Formation." In Spectral Evolution of Galaxies. Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4598-2_2.

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Ciardi, Benedetta. "Primordial Galaxy Formation and IGM Reionization." In The Evolution of Galaxies. Springer Netherlands, 2002. http://dx.doi.org/10.1007/978-94-017-3311-3_120.

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Conference papers on the topic "Bar formation, galaxy evolution"

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Zhang, Tianyu. "The Role of Dark Matter in Galaxy Formation and Evolution." In International Conference on Innovations in Applied Mathematics, Physics and Astronomy. SCITEPRESS - Science and Technology Publications, 2024. http://dx.doi.org/10.5220/0013077700004601.

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Sykes, Amber, Joshua Owen, Robert Jacklin, Richard C. Woollam, Danny Burkle, and Richard Barker. "Numerical Study to Investigate the Influence of Porous FeCO3 Layers on the CO2 Corrosion Rate of Carbon Steel." In CONFERENCE 2025. AMPP, 2025. https://doi.org/10.5006/c2025-00417.

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Abstract The formation of protective iron carbonate (FeCO3) corrosion product layers on X65 carbon steel has been investigated experimentally in high-temperature, high-pressure autoclave corrosion tests. Corrosion testing was performed in carbon dioxide (CO2)-saturated, 3 wt.% sodium chloride (NaCl) brine at an operating temperature of 80 °C and pressure of 5 bar. The evolution in corrosion rate and mass transfer processes during the formation of an FeCO3 layer were monitored using in-situ linear polarization resistance and electrochemical impedance spectroscopy. Over time, the precipitation o
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HUGHES, DAVID H., and ENRIQUE GAZTAÑAGA. "SIMULATED SUBMILLIMETRE GALAXY SURVEYS." In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0027.

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Fraternali, Filippo, Victor P. Debattista, and C. C. Popescu. "Gas Circulation and Galaxy Evolution." In HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458468.

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DUNLOP, JAMES S. "SUB-MM CLUES TO ELLIPTICAL GALAXY FORMATION." In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0002.

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Kaufmann, Tobias, James S. Bullock, Ari Maller, Taotao Fang, Robert Minchin, and Emmanuel Momjian. "Cold Cloud Infall and Galaxy Formation." In THE EVOLUTION OF GALAXIES THROUGH THE NEUTRAL HYDROGEN WINDOW. AIP, 2008. http://dx.doi.org/10.1063/1.2973568.

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DEVLIN, MARK J. "BLAST – A BALLOON-BORNE LARGE APERTURE SUBMILLIMETRE TELESCOPE." In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0010.

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WILNER, D. J. "SOME PROSPECTS FOR HIGH REDSHIFT GALAXY OBSERVATIONS WITH THE SUBMILLIMETER ARRAY." In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0009.

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ROBSON, IAN, WAYNE HOLLAND, and WILLIAM DUNCAN. "SCUBA–2, THE NEXT GENERATION, WIDE–FIELD SUBMILLIMETRE CAMERA FOR THE JCMT." In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0011.

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SMAIL, IAN, ROB IVISON, ANDREW BLAIN, and JEAN-PAUL KNEIB. "THE NATURE OF FAINT SUBMILLIMETER GALAXIES." In Implications for Galaxy Formation and Evolution. WORLD SCIENTIFIC, 2001. http://dx.doi.org/10.1142/9789812811738_0001.

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Reports on the topic "Bar formation, galaxy evolution"

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Bunker, A. J., and W. J. M. van Breugel. The Hy-Redshift Universe: Galaxy Formation and Evolution at High Redshift. Office of Scientific and Technical Information (OSTI), 1999. http://dx.doi.org/10.2172/793845.

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