Gotowa bibliografia na temat „Structure and evolution of the Galaxy”
Utwórz poprawne odniesienie w stylach APA, MLA, Chicago, Harvard i wielu innych
Spis treści
Zobacz listy aktualnych artykułów, książek, rozpraw, streszczeń i innych źródeł naukowych na temat „Structure and evolution of the Galaxy”.
Przycisk „Dodaj do bibliografii” jest dostępny obok każdej pracy w bibliografii. Użyj go – a my automatycznie utworzymy odniesienie bibliograficzne do wybranej pracy w stylu cytowania, którego potrzebujesz: APA, MLA, Harvard, Chicago, Vancouver itp.
Możesz również pobrać pełny tekst publikacji naukowej w formacie „.pdf” i przeczytać adnotację do pracy online, jeśli odpowiednie parametry są dostępne w metadanych.
Artykuły w czasopismach na temat "Structure and evolution of the Galaxy"
White, Simon. "The influence of halo evolution on galaxy structure". Proceedings of the International Astronomical Union 10, H16 (sierpień 2012): 371. http://dx.doi.org/10.1017/s1743921314011430.
Pełny tekst źródłaYee, H. K. C., M. J. Sawicki, R. G. Carlberg, H. Lin, S. L. Morris, D. R. Patton, G. D. Wirth i in. "The CNOC2 Field Galaxy Redshipt Survey". Highlights of Astronomy 11, nr 1 (1998): 460–63. http://dx.doi.org/10.1017/s153929960002178x.
Pełny tekst źródłaMaartens, Roy, José Fonseca, Stefano Camera, Sheean Jolicoeur, Jan-Albert Viljoen i Chris Clarkson. "Magnification and evolution biases in large-scale structure surveys". Journal of Cosmology and Astroparticle Physics 2021, nr 12 (1.12.2021): 009. http://dx.doi.org/10.1088/1475-7516/2021/12/009.
Pełny tekst źródłaNagai, Daisuke, Monique Arnaud, Sarthak Dasadia, Michael McDonald, Ikuyuki Mitsuishi i Andrea Morandi. "Cluster Physics & Evolution". Proceedings of the International Astronomical Union 11, A29B (sierpień 2015): 70–78. http://dx.doi.org/10.1017/s1743921316004543.
Pełny tekst źródłaConselice, Christopher J. "The Evolution of Galaxy Structure Over Cosmic Time". Annual Review of Astronomy and Astrophysics 52, nr 1 (18.08.2014): 291–337. http://dx.doi.org/10.1146/annurev-astro-081913-040037.
Pełny tekst źródłaGilmore, Gerard, i Rosemary F. G. Wyse. "Structure and Evolution of the Milky Way Galaxy". International Astronomical Union Colloquium 111 (1989): 83–102. http://dx.doi.org/10.1017/s0252921100011465.
Pełny tekst źródłaRobin, A. C., C. Reylé i D. Marshall. "Modelling the Galaxy from survey data". Proceedings of the International Astronomical Union 3, S248 (październik 2007): 443–49. http://dx.doi.org/10.1017/s1743921308019789.
Pełny tekst źródłaMazzei, P., A. Marino, R. Rampazzo, H. Plana, M. Rosado i L. Arias. "Galaxy evolution in groups". Astronomy & Astrophysics 610 (luty 2018): A8. http://dx.doi.org/10.1051/0004-6361/201731182.
Pełny tekst źródłaLinke, Laila, Patrick Simon, Peter Schneider, Thomas Erben, Daniel J. Farrow, Catherine Heymans, Hendrik Hildebrandt i in. "KiDS+VIKING+GAMA: Testing semi-analytic models of galaxy evolution with galaxy–galaxy–galaxy lensing". Astronomy & Astrophysics 640 (sierpień 2020): A59. http://dx.doi.org/10.1051/0004-6361/202038355.
Pełny tekst źródłaGilmore, Gerard, i Rodrigo Ibata. "Large Scale Galactic Structure". International Astronomical Union Colloquium 148 (1995): 258–66. http://dx.doi.org/10.1017/s0252921100022004.
Pełny tekst źródłaRozprawy doktorskie na temat "Structure and evolution of the Galaxy"
Machado, murtinheiras martins Andre. "Statistical analysis of large scale surveys for constraining the Galaxy evolution". Thesis, Besançon, 2014. http://www.theses.fr/2014BESA2026/document.
Pełny tekst źródłaThe formation and evolution of the thick disc of the Milky Way remain controversial. We made use of a population synthesis model of the Galaxy, the Besançon Galaxy Model (Robin et al. 2003), which can be used for data interpretation, study the Galactic structure and test different scenarios of Galaxy formation and evolution. We examined these questions by studying the shape and the metallicity distribution of the thin and thick disc using the population synthesis approach. We imposed on simulations observational errors and biases to make them directly comparable to observations. We corrected magnitudes and colors of stars, from the simulation, using an extinction model. The available extinction models do not always reproduce the exact quantity of extinction along the line of sight. A code to correct the distribution of extinction in distance along these lines have been developed and the corrected extinctions have been applied on model simulations. We studied the shape of the thin disc using photometric data at low latitudes from the SDSS-SEGUE survey. We compared qualitatively and quantitatively observations and simulations and try to constrain the Initial Mass Function. Using the spectroscopic survey SEGUE we selected Main Sequence Turnoff (MSTO) stars (Cheng et al 2012) and K giants to study the metallicity distribution of the thin and thick discs. We computed a distance for each star from the relation between effective temperatures and absolute magnitudes for the observed and simulated catalogs. These two catalogues have the same biases in distances, therefore are comparable. We developed a tool based on a MCMC-ABC method to determine the metallicity distribution and study the correlations between the fitted parameters. We confirmed a radial metallicity gradient of -0.079 ± 0.015 dex kpc−1 for the thin disc. We obtained a solar neighborhood metallicity of the thick disc of -0.47 ± 0.03 dex similar to previous studies and the thick disc shows no gradient but the data are compatible with an inner positive gradient followed by a outer negative one. Furthermore, we have applied the developed tools to the Gaia-ESO spectroscopic survey and computed the metallicity distribution of F/G/K stars in the thin and thick disc assuming a two epoch formation for the thick disc of the Milky Way. We obtained a local metallicity in the thick disc of -0.23 ± 0.04 dex slightly higher than the one obtained with SEGUE but in agreement with Adibekyan et al. (2013) and a radial metallicity gradient for the thick disc in agreement with our previous analysis of SEGUE data and the literature. The local metallicity is in fair agreement with literature at the 3σ level but because the GES data is an internal release under testing further analysis with more data and better calibrations have to be done. The existence of a flat gradient in the thick disc can be a consequence of an early formation from a highly turbulent homogeneous well mixed gas, unless it has suffered heavy radial mixing later on
Cole, Shaun. "Evolution of large scale structure and galaxy formation". Thesis, University of Cambridge, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.315745.
Pełny tekst źródłaMajewski, Steven R., Ricardo P. Schiavon, Peter M. Frinchaboy, Carlos Allende Prieto, Robert Barkhouser, Dmitry Bizyaev, Basil Blank i in. "The Apache Point Observatory Galactic Evolution Experiment (APOGEE)". IOP PUBLISHING LTD, 2017. http://hdl.handle.net/10150/625493.
Pełny tekst źródłaDurkalec, Anna. "Properties and evolution of galaxy clustering at 2". Thesis, Aix-Marseille, 2014. http://www.theses.fr/2014AIXM4758/document.
Pełny tekst źródłaThis thesis focuses on the study of the properties and evolution of galaxy clustering for galaxies in the redshift range 22. I was able to measure the spatial distribution of a general galaxy population at redshift z~3 for the first time with a high accuracy. I quantified the galaxy clustering by estimating and modelling the projected (real-space) two-point correlation function, for a general population of 3022 galaxies. I extended the clustering measurements to the luminosity and stellar mass-selected sub-samples. My results show that the clustering strength of the general galaxy population does not change significantly from redshift z~3.5 to z~2.5, but in both redshift ranges more luminous and more massive galaxies are more clustered than less luminous (massive) ones. Using the halo occupation distribution (HOD) formalism I measured an average host halo mass at redshift z~3 significantly lower than the observed average halo masses at low redshift. I concluded that the observed star-forming population of galaxies at z~3 might have evolved into the massive and bright (Mr<-21.5) galaxy population at redshift z=0. Also, I interpret clustering measurements in terms of a linear large-scale galaxy bias. I find it to be significantly higher than the bias of intermediate and low redshift galaxies. Finally, I computed the stellar-to-halo mass ratio (SHMR) and the integrated star formation efficiency (ISFE) to study the efficiency of star formation and stellar mass assembly. I find that the integrated star formation efficiency is quite high at ~16% for the average galaxies at z~3
Legrand, Louis. "Large surveys : from galaxy evolution to cosmological probes". Thesis, université Paris-Saclay, 2020. http://www.theses.fr/2020UPASP023.
Pełny tekst źródłaLarge galaxy surveys are like open windows on our Universe: they provide precious insights on its components and on its evolution. On the one hand, pencil surveys go deep into the cosmos to explore the formation and evolution of galaxies. On the other hand, wide surveys are mapping the distribution of matter on large scales to understand the nature of dark energy and dark matter.During my thesis, I explore the capabilities of these large surveys to address the following questions:1. What are the main drivers of galaxy evolution? 2. What improvements on our knowledge of the Universe will be brought by upcoming wide galaxy surveys? Using precise galaxy stellar-mass function measurements in the COSMOS field, I first determine the stellar-to-halo mass relation through a parametric abundance matching technique. Thanks to the completeness of the COSMOS survey from z ~ 0.2 to z ~ 5, I obtain for the first time this relation over such a large redshift range from a single coherent sample.I find that the ratio of stellar-to-halo mass content peaks at a characteristic halo mass which increases up to z = 2.3 and remains flat up to z = 4.This steady increase of the characteristic halo mass questions the role of cold gas inflows as drivers of galaxy formation at high redshift.To address this question, I link observations of the cold molecular gas content in galaxies up to z = 4 to the evolution of the dark matter halo mass. I find that the joint evolution of cold gas mass fraction and halo mass is in agreement with the hypothesis of cold gas inflows being responsible of efficient galaxy formation at high redshift.With the scope of maximising the cosmological power of next generation spectroscopic surveys, I show that a novel cosmological observable, the angular redshift fluctuations (ARF) will provide complementary cosmological information in addition to the standard angular galaxy clustering. Due to its distinct sensitivity to the peculiar velocity field, I find that the cosmological and galaxy bias parameters express different degeneracies when inferred from ARF or from angular galaxy clustering.As such, combining both observables breaks these degeneracies and greatly decreases the marginalised uncertainties, by a factor of at least two on most parameters in the ^CDM and wCDM models.As part of the Euclid collaboration, I then investigate the cosmological power of the upcoming Euclid survey, which will offer us an exquisite measurement of the matter distributions on the full extra-galactic sky.In order to fully exploit all the potential of the Euclid survey it is crucial to combine it with upcoming CMB surveys.I use the Fisher formalism to forecast the benefits of performing a joint analysis of CMB probes with Euclid main probes (weak lensing and galaxy clustering). I test both the standard cosmological model, ^CDM, and its extensions, and show that CMB will improve the constraints by a factor two on most cosmological parameters, and most notably on dark energy modified models which are of key interest for Euclid
Hatzidimitriou, D. "The evolution and geometry of the oouter parts of the Small Magellanic Cloud". Thesis, University of Edinburgh, 1989. http://ethos.bl.uk/OrderDetails.do?uin=uk.bl.ethos.234097.
Pełny tekst źródłaLaporte, Chervin F. P., Facundo A. Gómez, Gurtina Besla, Kathryn V. Johnston i Nicolas Garavito-Camargo. "Response of the Milky Way's disc to the Large Magellanic Cloud in a first infall scenario". OXFORD UNIV PRESS, 2018. http://hdl.handle.net/10150/626276.
Pełny tekst źródłaKruk, Sandor J. "Evolution of barred galaxies and associated structures". Thesis, University of Oxford, 2018. http://ora.ox.ac.uk/objects/uuid:34cc9283-a386-464f-b9ae-1d4e3b4fdf77.
Pełny tekst źródłaLaigle, Clotilde. "Observational and theoretical constraints on galaxy evolution at high redshift". Thesis, Paris 6, 2016. http://www.theses.fr/2016PA066343.
Pełny tekst źródłaI present in this thesis new constraints on galaxy formation and evolution while studying the galaxy mass growth and the co-evolution of the cosmic web and the embedded galaxies, from the epoch of cosmic dawn to today.To do so, I first created a new photometric catalog on the COSMOS field with precise photometric redshifts allowing to probe accurately the high-redshift Universe. I analyze this survey while relying heavily on comparisons with virtual galaxy surveys produced from state-of-the- art cosmological hydrodynamical simulations, which capture all our current knowledge of galaxy formation and evolution.From this comparative analysis, in the first part of my thesis I show that the redshift evolution of galaxy properties is reasonably well understood when invoking mass-dependent processes (AGN and stellar feed- back). I highlight also the effect of simplifying assumptions inherent to our observational methods, which bias the physical properties computed from galaxy photometry.Galaxies and haloes are embedded in the cosmic web, an intricate large-scale structure of walls, filaments and nodes. In the second part of my thesis, I show how galaxies and dark haloes gain their angular momentum from the large-scale flow, implying that some of their properties depend on their anisotropic filamentary environment. I then extract the filamentary structure from the observed photometric catalog and measure the dependence of galaxy properties to the anisotropic environment. I find mass and colour gradients towards the filaments. In turn it emerges that galaxy masses and angular momenta are two dependent quantities impacted by their anisotropic environment
Roldán, Carlos Antonio Calcáneo. "The evolution of dark matter substructure". Thesis, Durham University, 2001. http://etheses.dur.ac.uk/4232/.
Pełny tekst źródłaKsiążki na temat "Structure and evolution of the Galaxy"
S, Mulchaey John, Dressler Alan Michael i Oemler Augustus 1945-, red. Clusters of galaxies: Probes of cosmological structure and galaxy evolution. Cambridge: Cambridge University Press, 2004.
Znajdź pełny tekst źródłaGuillermo Haro Conference on Astrophysics (3rd 1999 Puebla, Pue., Mexico). Cosmic evolution and galaxy formation: Structure, interactions, and feedback : the 3rd Guillermo Haro Astrophysics Conference. San Francisco, Calif: Astronomical Society of the Pacific, 2000.
Znajdź pełny tekst źródłaGiuseppina, Fabbiano, Harvard-Smithsonian Center for Astrophysics i United States. National Aeronautics and Space Administration., red. The evolution of gas and stars in the merger galaxy NGC 1316 (Fornax A). Cambridge, Mass: Harvard-Smithsonian Center for Astrophysics, 1998.
Znajdź pełny tekst źródłaWeinzirl, Timothy. Probing Galaxy Evolution by Unveiling the Structure of Massive Galaxies Across Cosmic Time and in Diverse Environments. Cham: Springer International Publishing, 2015. http://dx.doi.org/10.1007/978-3-319-06959-3.
Pełny tekst źródła1956-, Clemens Dan P., Shah Ronak Y, Brainerd Tereasa G. 1964- i Boston University. Institute for Astrophysical Research., red. Milky Way surveys: The structure and evolution of our Galaxy : the fifth Boston University Astrophysics conference : proceedings of a meeting held in Boston, Massachusetts, 15-17 June 2003. San Francisco: Astronomical Society of the Pacific, 2004.
Znajdź pełny tekst źródłaVan den Bosch, Frank, 1969- i White S, red. Galaxy formation and evolution. Cambridge: Cambridge University Press, 2010.
Znajdź pełny tekst źródłaGalaxy formation and evolution. Berlin: Springer, 2005.
Znajdź pełny tekst źródłaSpinrad, Hyron. Galaxy formation and evolution. Berlin, Germany: Springer, 2005.
Znajdź pełny tekst źródłaBender, Ralf, i Roger L. Davies, red. New Light on Galaxy Evolution. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0229-9.
Pełny tekst źródłaKippenhahn, Rudolf, Alfred Weigert i Achim Weiss. Stellar Structure and Evolution. Berlin, Heidelberg: Springer Berlin Heidelberg, 2012. http://dx.doi.org/10.1007/978-3-642-30304-3.
Pełny tekst źródłaCzęści książek na temat "Structure and evolution of the Galaxy"
Grosbøl, Preben. "Spiral Structure and Galaxy Evolution". W Astrophysics and Space Science Library, 105–10. Dordrecht: Springer Netherlands, 1988. http://dx.doi.org/10.1007/978-94-009-2919-7_13.
Pełny tekst źródłaNavarro, Julio F. "The Structure of Cold Dark Matter Halos". W New Light on Galaxy Evolution, 255–58. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0229-9_38.
Pełny tekst źródłaVillumsen, Jens Verner. "Evolution of the Vertical Structure of Galactic Disks". W The Milky Way Galaxy, 491–92. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5291-1_94.
Pełny tekst źródłaBurkert, A. "The Structure of Dark Matter Halos in Dwarf Galaxies". W New Light on Galaxy Evolution, 175–78. Dordrecht: Springer Netherlands, 1996. http://dx.doi.org/10.1007/978-94-009-0229-9_25.
Pełny tekst źródłaValentijn, Edwin A. "Are Cooling Flows Governing E-Galaxy Evolution?" W Structure and Dynamics of Elliptical Galaxies, 433–34. Dordrecht: Springer Netherlands, 1987. http://dx.doi.org/10.1007/978-94-009-3971-4_59.
Pełny tekst źródłaHidalgo, Sebastian L., Antonio Aparicio i David Martínez-Delgado. "The Extended Structure of the Phoenix Dwarf Galaxy". W The Evolution of Galaxies, 301–4. Dordrecht: Springer Netherlands, 2003. http://dx.doi.org/10.1007/978-94-017-3315-1_57.
Pełny tekst źródłavan der Laan, H., P. Katgert i M. J. A. Oort. "Radio Galaxy Populations: A Progress Report". W Structure and Evolution of Active Galactic Nuclei, 437–45. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4562-3_25.
Pełny tekst źródłaVan Loon, Jacco. "Structure and Evolution of the Inner Milky Way Galaxy". W The Evolution of Galaxies, 313–16. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-017-3313-7_69.
Pełny tekst źródłaMeurs, E. J. A. "Towards the Luminosity Function of Seyfert Galaxy Nuclei". W Structure and Evolution of Active Galactic Nuclei, 641–44. Dordrecht: Springer Netherlands, 1986. http://dx.doi.org/10.1007/978-94-009-4562-3_66.
Pełny tekst źródłaMarconi, M., I. Musella, M. Di Criscienzo, M. Cignoni, M. Dall’Ora, V. Ripepi, G. Bono i in. "STREGA@VST: Structure and Evolution of the Galaxy". W Astrophysics and Space Science Proceedings, 139–43. Cham: Springer International Publishing, 2016. http://dx.doi.org/10.1007/978-3-319-19330-4_22.
Pełny tekst źródłaStreszczenia konferencji na temat "Structure and evolution of the Galaxy"
Kelvin, Lee, Simon Driver, Aaron Robotham, David Hill, Ewan Cameron, Victor P. Debattista i C. C. Popescu. "Exploring Galaxy Formation and Evolution via Structural Decomposition". W HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458501.
Pełny tekst źródłaBouchard, Antoine, Sarah Blyth, W. J. G. de Blok, Benne Holwerda i Kurt van der Heyden. "The Environmental Impact on Galaxy Evolution: Highlighting the Structure of the Local Cosmic Web". W Panoramic Radio Astronomy: Wide-field 1-2 GHz research on galaxy evolution. Trieste, Italy: Sissa Medialab, 2010. http://dx.doi.org/10.22323/1.089.0053.
Pełny tekst źródłaPan, Jing, Yijie Shen, Hao Wang i Qiang Liu. "Galaxy waves: 3D inhomogeneous auto-accelerating beams". W CLEO: Science and Innovations. Washington, D.C.: Optica Publishing Group, 2022. http://dx.doi.org/10.1364/cleo_si.2022.sf3i.8.
Pełny tekst źródłaStanghellini, Carlo. "Radio galaxy Evolution". W First MCCT-SKADS Training School. Trieste, Italy: Sissa Medialab, 2008. http://dx.doi.org/10.22323/1.059.0015.
Pełny tekst źródłaSilk, Joseph, i Rychard Bouwens. "Simulating galaxy evolution". W AFTER THE DARK AGES. ASCE, 1999. http://dx.doi.org/10.1063/1.58639.
Pełny tekst źródłaMadore, Barry F. "GALEX: Galaxy Evolution Explorer". W THE SPECTRAL ENERGY DISTRIBUTIONS OF GAS-RICH GALAXIES: Confronting Models with Data; International Workshop. AIP, 2005. http://dx.doi.org/10.1063/1.1913948.
Pełny tekst źródłaMartin, Christopher, Thomas Barlow, William Barnhart, Luciana Bianchi, Brian K. Blakkolb, Dominique Bruno, Joseph Bushman i in. "The Galaxy Evolution Explorer". W Astronomical Telescopes and Instrumentation, redaktorzy J. Chris Blades i Oswald H. W. Siegmund. SPIE, 2003. http://dx.doi.org/10.1117/12.460034.
Pełny tekst źródłaTonnesen, Stephanie. "Environmentally-Driven Galaxy Evolution". W Frank N. Bash Symposium 2011: New Horizons in Astronomy. Trieste, Italy: Sissa Medialab, 2012. http://dx.doi.org/10.22323/1.149.0008.
Pełny tekst źródłaPage, M. J., F. J. Carrera, J. A. Stevens, A. Comastri, L. Angelini i M. Cappi. "QSO winds and galaxy evolution". W X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Conference. AIP, 2010. http://dx.doi.org/10.1063/1.3475264.
Pełny tekst źródłaFraternali, Filippo, Victor P. Debattista i C. C. Popescu. "Gas Circulation and Galaxy Evolution". W HUNTING FOR THE DARK: THE HIDDEN SIDE OF GALAXY FORMATION. AIP, 2010. http://dx.doi.org/10.1063/1.3458468.
Pełny tekst źródłaRaporty organizacyjne na temat "Structure and evolution of the Galaxy"
Arraki, Kenza Sigrid. Evolution of dwarf galaxy properties in local group environments. Office of Scientific and Technical Information (OSTI), maj 2016. http://dx.doi.org/10.2172/1491856.
Pełny tekst źródłaZhang, Yuanyuan. Looking Wider and Further: The Evolution of Galaxies Inside Galaxy Clusters. Office of Scientific and Technical Information (OSTI), styczeń 2016. http://dx.doi.org/10.2172/1248222.
Pełny tekst źródłaBunker, A. J., i W. J. M. van Breugel. The Hy-Redshift Universe: Galaxy Formation and Evolution at High Redshift. Office of Scientific and Technical Information (OSTI), listopad 1999. http://dx.doi.org/10.2172/793845.
Pełny tekst źródłaMeyer, B. S., i D. N. Schramm. General constraints on the age and chemical evolution of the Galaxy. Office of Scientific and Technical Information (OSTI), maj 1986. http://dx.doi.org/10.2172/5797647.
Pełny tekst źródłaEspaña Fontán, Paula, i Maria Angeles Gomez Flechoso. Effects of the orbit orientation on the evolution of dwarf satellite galaxies. Fundación Avanza, maj 2023. http://dx.doi.org/10.60096/fundacionavanza/2492022.
Pełny tekst źródłaPiacentine, J. Detection of Galaxy Clusters with the XMM-Newton Large Scale Structure Survey. Office of Scientific and Technical Information (OSTI), wrzesień 2004. http://dx.doi.org/10.2172/833122.
Pełny tekst źródłaKeller, Christopher J. Analysis of Pacific Enroute Structure in Support of C-5M Super Galaxy. Fort Belvoir, VA: Defense Technical Information Center, czerwiec 2015. http://dx.doi.org/10.21236/ada619564.
Pełny tekst źródłaArnold, Frances H. Evolution by Structure-Based Protein Recombination. Fort Belvoir, VA: Defense Technical Information Center, czerwiec 2003. http://dx.doi.org/10.21236/ada417404.
Pełny tekst źródłaMartin, J. E., J. P. Wilcoxon i R. A. Anderson. Evolution of structure during phase transitions. Office of Scientific and Technical Information (OSTI), marzec 1996. http://dx.doi.org/10.2172/238582.
Pełny tekst źródłaHoversten, Erik A. Galaxy Evolution Insights from Spectral Modeling of Large Data Sets from the Sloan Digital Sky Survey. Office of Scientific and Technical Information (OSTI), październik 2007. http://dx.doi.org/10.2172/935485.
Pełny tekst źródła