Auswahl der wissenschaftlichen Literatur zum Thema „Comets Dynamics“
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Zeitschriftenartikel zum Thema "Comets Dynamics"
Carusi, A., und G. B. Valsecchi. „Dynamics of Comets“. Symposium - International Astronomical Union 152 (1992): 255–68. http://dx.doi.org/10.1017/s0074180900091245.
Der volle Inhalt der QuelleZheng, J. Q., M. J. Valtonen, S. Mikkola und H. Rickman. „Dynamics and orbital evolution of Oort cloud comets“. Symposium - International Astronomical Union 172 (1996): 209–12. http://dx.doi.org/10.1017/s007418090012738x.
Der volle Inhalt der QuelleFernández, Julio A. „Dynamics of Comets: Recent Developments and New Challenges“. Symposium - International Astronomical Union 160 (1994): 223–40. http://dx.doi.org/10.1017/s0074180900046568.
Der volle Inhalt der QuelleNeslušan, L. „Dynamics of comets in the collapsing protosolar nebula“. International Astronomical Union Colloquium 173 (1999): 45–50. http://dx.doi.org/10.1017/s0252921100031225.
Der volle Inhalt der QuelleBorinskaya, Sofya, Katrina B. Velle, Kenneth G. Campellone, Arthur Talman, Diego Alvarez, Hervé Agaisse, Yi I. Wu, Leslie M. Loew und Bruce J. Mayer. „Integration of linear and dendritic actin nucleation in Nck-induced actin comets“. Molecular Biology of the Cell 27, Nr. 2 (15.01.2016): 247–59. http://dx.doi.org/10.1091/mbc.e14-11-1555.
Der volle Inhalt der QuelleS. Najm, Rasha, Salman Z. Khalaf und Khaleel I. Abood. „X-Ray Emission Spectroscopy Analysis for Near-Asteroid Belt of Atmospheric of the Comets“. Iraqi Journal of Physics 20, Nr. 3 (01.09.2022): 86–97. http://dx.doi.org/10.30723/ijp.v20i3.1006.
Der volle Inhalt der QuelleMysen, Eirik. „Rotational dynamics of subsolar sublimating triaxial comets“. Planetary and Space Science 52, Nr. 10 (August 2004): 897–907. http://dx.doi.org/10.1016/j.pss.2004.04.001.
Der volle Inhalt der QuelleEmel'yanenko, V. V. „Dynamics of periodic comets and meteor streams“. Celestial Mechanics and Dynamical Astronomy 54, Nr. 1-3 (1992): 91–110. http://dx.doi.org/10.1007/bf00049546.
Der volle Inhalt der QuelleHaghighipour, N., T. I. Maindl, C. Schäfer, R. Speith und R. Dvorak. „Triggering Comet-Like Activity of Main Belt Comets“. Proceedings of the International Astronomical Union 10, S318 (August 2015): 135–41. http://dx.doi.org/10.1017/s1743921315009680.
Der volle Inhalt der QuelleFernández, J. A., und T. Gallardo. „From the Oort cloud to Halley-type comets“. International Astronomical Union Colloquium 173 (1999): 327–38. http://dx.doi.org/10.1017/s0252921100031638.
Der volle Inhalt der QuelleDissertationen zum Thema "Comets Dynamics"
De, Biasi Alice. „Tidal Effects on the Oort Cloud Comets and Dynamics of the Sun in the Spiral Arms of the Galaxy“. Doctoral thesis, Università degli studi di Padova, 2014. http://hdl.handle.net/11577/3423732.
Der volle Inhalt der QuelleIl Sistema Solare è una struttura con una dinamica complessa e non isolata da quella galattica. In particolare la riserva cometaria del nostro sistema planetario, la nube di Oort, a causa della sua periferica collocazione all’interno del Sistema Solare, risulta estremamente sensibile all'ambiente galattico circostante. In questo contesto, le crescenti evidenze di una possibile migrazione del Sole, aprono un nuovo scenario di indagine relativo ai cambiamenti che tale migrazione potrebbe indurre sul moto cometario. Seguendo un filone di ricerca già tracciato, abbiamo identificato nella struttura a spirale la principale perturbazione in grado di produrre un efficace effetto migratorio per il Sole. Ampliando il classico modello di Lin & Shu con una modellizzazione 3D per i bracci a spirale considerati in regime transiente, siamo stati in grado di verificare la compatibilità tra tale perturbazione e un moto solare attraverso il disco, in accordo con i vincoli di posizione, velocità e metallicità imposti dalla attuale condizione della nostra stella. Malgrado i maggiori perturbatori della nube di Oort, i passaggi stellari ravvicinati e il campo mareale della Galassia, siano entrambi potenzialmente sensibili alla variazione di ambiente galattico che una migrazione solare comporta, abbiamo concentrato il nostro studio unicamente sulla marea galattica. La perturbazione dovuta alla spirale, è stata incorporata nello studio dei moti cometari, sia attraverso l’introduzione della migrazione solare, che come effetto diretto sulle comete grazie alla presenza della componente non assisimmetrica nel campo mareale. I risultati mostrano un’influenza significativa della spirale, in particolar modo sulla popolazione cometaria del guscio più esterno della nube, per la quale si sono registrati tassi di immissione cometaria 3 volte maggiori rispetto al caso senza tale perturbazione. La spirale sembra rinforzare l’azione della componente piana della marea, producendo infatti le maggiori variazioni sui perieli cometari in corrispondenza di orbite con inclinazioni moderate rispetto al piano galattico. Si è inoltre rilevato che il picco di immissione cometaria si trova in corrispondenza di distanze galattiche per il Sole comprese tra 6 e 7 kpc. Se tale evidenza fosse confermata anche da campioni cometari più realistici, potrebbe comportare un vincolo ulteriore alla definizione della zona di abitabilità galattica (GHZ). In particolare, regioni del disco non attualmente precluse alla formazione della vita, potrebbero risultare inadatte allo sviluppo della stessa per un rischio di impatto cometario troppo elevato
Gkotsinas, Anastasios. „On the pristine nature of cometary nuclei : coupled modeling of their thermal and dynamical evolution“. Electronic Thesis or Diss., Lyon 1, 2023. http://www.theses.fr/2023LYO10144.
Der volle Inhalt der QuelleComets are a population of small Solar System bodies, often described as the most primitive population in our Solar System, holding valuable information on its formation and evolution. Formed early, at the same time as the giant planets, in the outer parts of the protoplanetary disk and scattered outwards shortly after their formation towards distant and cold reservoirs, they are considered to have preserved their primordial composition and properties to a great extent. However, the level of this primitive nature has started to be reevaluated recently, as a growing body of observational evidence and an important number of theoretical studies are suggesting the possibility of thermally-induced alterations before their return to the inner parts of the Solar System, where they are usually studied and observed. In this context, our work aims to examine the level of the primitive nature of different cometary families in our Solar System. To do so, we developed a dedicated thermal evolution model, designed for an efficient coupling to N-body simulations, tracking the long-term orbital evolution of planetesimals, originating in the outer parts of the protoplanetary disk and evolving into planetary-crossing orbits after a prolonged stay in outer Solar System reservoirs. Our results reveal the possibility of thermal processing, affecting mainly the primordial condensed hyper-volatile content and on a lesser extent the primordial moderately-volatile and amorphous water ice content, during the early phases of a comet's lifetime. A comparative study is indicating that long-period comets are expected to be the least altered population. Intense, yet sporadic, activity is also recorded in the planetary region, as comets return in the inner Solar System, compatible with the current observables on the Centaur population. These results indicate that the thermal evolution of cometary nuclei is inextricably related to their orbital evolution. They are also indicating that the cometary activity observed in the inner parts of the Solar System is very likely triggered from thermally processed subsurface layers, highlighting the necessity of considering the past evolutionary history of comets when interpreting the current observations in a broader context
Volk, Kathryn Margaret. „Dynamical studies of the Kuiper belt and the Centaurs“. Thesis, The University of Arizona, 2013. http://pqdtopen.proquest.com/#viewpdf?dispub=3560868.
Der volle Inhalt der QuelleThe Kuiper belt is a population of small bodies located outside Neptune's orbit. The observed Kuiper belt objects (KBOs) can be divided into several subclasses based on their dynamical structure. I construct models for these subclasses and use numerical integrations to investigate their long-term evolution. I use these models to quantify the connection between the Kuiper belt and the Centaurs (objects whose orbits cross the orbits of the giant planets) and the short-period comets in the inner solar system. I discuss how these connections could be used to determine the physical properties of KBOs and what future observations could conclusively link the comets and Centaurs to specific Kuiper belt subclasses.
The Kuiper belt's structure is determined by a combination of long-term evolution and its formation history. The large eccentricities and inclinations of some KBOs and the prevalence of KBOs in mean motion resonances with Neptune are evidence that much of the Kuiper belt's structure originated during the solar system's epoch of giant planet migration; planet migration can sculpt the Kuiper belt's scattered disk, capture objects into mean motion resonances, and dynamically excite KBOs. Different models for planet migration predict different formation locations for the subclasses of the Kuiper belt, which might result in different size distributions and compositions between the subclasses; the high-inclination portion of the classical Kuiper belt is hypothesized to have formed closer to the Sun than the low-inclination classical Kuiper belt. I use my model of the classical Kuiper belt to show that these two populations remain largely dynamically separate over long timescales, so primordial physical differences could be maintained until the present day.
The current Kuiper belt is much less massive than the total mass required to form its largest members. It must have undergone a mass depletion event, which is likely related to planet migration. The Haumea collisional family dates from the end of this process. I apply long-term evolution to family formation models and determine how they can be observationally tested. Understanding the Haumea family's formation could shed light on the nature of the mass depletion event.
Heisler, Julia. „Dynamical influences on the comets of the Oort Cloud“. Thesis, Massachusetts Institute of Technology, 1986. http://hdl.handle.net/1721.1/15186.
Der volle Inhalt der QuelleHu, Hongyao. „Atmospheres of comets: Gas dynamic models and inference of kinematic parameters“. Diss., The University of Arizona, 1991. http://hdl.handle.net/10150/185429.
Der volle Inhalt der QuelleConrad, Michael Curt. „COMET: CONSTRAINED OPTIMIZATION OF MULTIPLE-DIMENSIONS FOR EFFICIENT TRAJECTORIES“. DigitalCommons@CalPoly, 2011. https://digitalcommons.calpoly.edu/theses/666.
Der volle Inhalt der QuellePujolàs, Fons Pau Salvador. „Essays on International Trade and Firm Dynamics“. Doctoral thesis, Universitat Autònoma de Barcelona, 2013. http://hdl.handle.net/10803/120540.
Der volle Inhalt der QuelleThe first chapter of this Thesis is entitled Trade Patterns, Income Differences and Gains From Trade and is coauthored with my colleague Wyatt J. Brooks. Quantifying the gains from international trade is an area of research that has been widely studied using a variety of trade models. At the same time, it has been shown that nonhomotheticities are useful for matching the systematic patterns of trade present in disaggregated trade data. We bring these two literatures together to ask how nonhomotheticities affect our predictions for gains from trade. To do so, we develop a N-country trade model that exactly matches bilateral trade, population, GDP per capita and within country income inequality for many countries. We include nonhomotheticities to match patterns of trade between rich and poor countries that we observe in highly disaggregated trade data. We then make use of the results from Arkolakis, Costinot, and Rodriguez-Clare (2012), which gives a simple formula for gains from trade in a large class of homothetic models, including a version of our model with the nonhomotheticity removed. Our main finding is that homothetic models underestimate gains from trade in countries with small populations and low productivities, and overestimate gains in countries with large populations and high productivities. The homothetic model overestimates the gains from being open to trade in the U.S. and Japan by 14% and 22%, and underestimates them in Spain and Italy by 24% and 14%. The second chapter of this Thesis is entitled Measured Productivity and International Trade: An Unresolved Puzzle. Using correct models of firm dynamics when analyzing the impact of trade is key in order to fully understand what are the effects to the supply side of the economy when it engages into trade. There are several models of trade that try to understand the role of trade and firm dynamics, but there is one that is most used by trade economists: the Melitz model (2003). This model explains several features of the data. In particular, it aims to explain why more productive firms export. It is a common agreement among economists that the model is well suited in order to explain these patterns. In this chapter we ask: is it? In particular, we show that measuring productivity in the model's outcome as it is done in the data may lead to some surprising results regarding what more productive firms do: they may be the non-exporters. The third chapter of this Thesis is entitled Distortions, Productivity, and Idiosyncratic Shocks and is coauthored with my professor José María Da Rocha. We consider policy distortions in a model where plants face idiosyncratic productivity shocks that evolve following a Brownian motion. Introducing idiosyncratic shocks into the model implies that plants have non-constant operating profits and as a result there is an endogenous exit margin and incumbent plants must decide in each period whether or not to remain in the industry. By using the forward Kolmogorov equation, we analytically characterize the Stationary Equilibrium. Our main contribution is to show that if a model is being calibrated/estimated without idiosyncratic shocks, where plants face constant productivity over time and the exit rate is exogenous to fit data generated from a model with shocks and endogenous entry, TFP distortions will be overestimated.
Beaver, David Ian. „Presupposition and assertion in dynamic semantics : Part (I) The presupposition : a critical review of presupposition theory ; Part (II) The assertion : what comes first in dynamic semantics“. Thesis, University of Edinburgh, 1995. http://hdl.handle.net/1842/10767.
Der volle Inhalt der QuelleDUVET, LUDOVIC. „Instrumentation pour l'etude in-situ des atmospheres neutres et ionises planetaires et cometaires : idm (ion dynamics monitor) et cops (comet pressure sensor)“. Paris 6, 2001. http://www.theses.fr/2001PA066296.
Der volle Inhalt der QuelleTsoumpra, Natalia. „Comic leadership and power dynamics in Aristophanes“. Thesis, University of Oxford, 2013. http://ora.ox.ac.uk/objects/uuid:1b3d4779-609e-4638-81f2-2e7f0d410477.
Der volle Inhalt der QuelleBücher zum Thema "Comets Dynamics"
The dynamics of Halley-type comets. Manchester: University of Manchester, 1994.
Den vollen Inhalt der Quelle findenChambers, John Eric. The dynamics of Halley-type comets. Manchester: University of Manchester, 1994.
Den vollen Inhalt der Quelle findenCarusi, Andrea, und Giovanni B. Valsecchi, Hrsg. Dynamics of Comets: Their Origin and Evolution. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5400-7.
Der volle Inhalt der QuelleFernández, J. A. Comets: Nature, dynamics, origin, and their cosmogonical relevance. Dordrecht, The Netherlands: Springer, 2005.
Den vollen Inhalt der Quelle findenComets: Nature, dynamics, origin, and their cosmogonical relevance. Dordrecht, Netherlands: Springer, 2005.
Den vollen Inhalt der Quelle findenYabushita, Shin, und Jacques Henrard, Hrsg. Dynamics of Comets and Asteroids and Their Role in Earth History. Dordrecht: Springer Netherlands, 1998. http://dx.doi.org/10.1007/978-94-017-1321-4.
Der volle Inhalt der Quelle1946-, Carusi Andrea, und Valsecchi Giovanni B. 1951-, Hrsg. Dynamics of comets: Their origin and evolution : proceedings of the 83rd Colloquium of the International Astronomical Union, held in Rome, Italy, 11-15 June 1984. Dordrecht, Holland: D. Reidel Pub. Co., 1985.
Den vollen Inhalt der Quelle findenInternational Astronomical Symposium (1992 Pléneuf-Val-André, France). Interactions between physics and dynamics of solar system bodies: Proceedings of the International Astronomical Symposium held in Pléneuf-Val-André (France) from June 21 to June 28, 1992. Dordrecht: Kluwer Academic Publishers, 1993.
Den vollen Inhalt der Quelle finden1936-, Yabushita Shin, und Henrard J, Hrsg. Dynamics of comets and asteroids and their role in earth history: Proceedings of a workshop held at the Dynic Astropark 'Ten-Kyu-Kan', August 14-18, 1997. Dordrecht, The Netherlands: Kluwer Academic, 1998.
Den vollen Inhalt der Quelle findenUnited States. National Aeronautics and Space Administration., Hrsg. The kinetics and dynamics of Halley's comet. Ann Arbor, MI: Space Physics Research Laboratory, Dept. of Atmospheric, Oceanic and Space Sciences, University of Michigan, 1994.
Den vollen Inhalt der Quelle findenBuchteile zum Thema "Comets Dynamics"
Milani, Andrea. „The Dynamics of the Trojan Asteroids“. In Asteroids, Comets, Meteors 1993, 159–74. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1148-5_12.
Der volle Inhalt der QuelleRemy, F., und F. Mignard. „Stellar Perturbations on Comets“. In Dynamics of Comets: Their Origin and Evolution, 97–104. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5400-7_8.
Der volle Inhalt der QuelleFernández, Julio A. „Dynamics of Comets: Recent Developments and New Challenges“. In Asteroids, Comets, Meteors 1993, 223–40. Dordrecht: Springer Netherlands, 1994. http://dx.doi.org/10.1007/978-94-011-1148-5_16.
Der volle Inhalt der QuelleNakamura, Tsuko, und Makoto Yoshikawa. „Invisible Comets On Evolutionary Track Of Short-Period Comets“. In Dynamics and Evolution of Minor Bodies with Galactic and Geological Implications, 261–66. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2743-1_22.
Der volle Inhalt der QuelleHughes, David W. „The Transition Between Long Period Comets, Short Period Comets and Meteoroid Streams“. In Dynamics of Comets: Their Origin and Evolution, 129–42. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5400-7_11.
Der volle Inhalt der QuelleRickman, Hans. „Interrelations between Comets and Asteroids“. In Dynamics of Comets: Their Origin and Evolution, 149–72. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5400-7_13.
Der volle Inhalt der QuelleYeomans, D. K. „Cometary Orbital Dynamics and Astrometry“. In Comets in the Post-Halley Era, 3–17. Dordrecht: Springer Netherlands, 1991. http://dx.doi.org/10.1007/978-94-011-3378-4_1.
Der volle Inhalt der QuelleKoon, W. S., M. W. Lo, J. E. Marsden und S. D. Ross. „Resonance and Capture of Jupiter Comets“. In Dynamics of Natural and Artificial Celestial Bodies, 27–38. Dordrecht: Springer Netherlands, 2001. http://dx.doi.org/10.1007/978-94-017-1327-6_3.
Der volle Inhalt der QuelleKresák, Ľubor. „The Aging and Lifetimes of Comets“. In Dynamics of Comets: Their Origin and Evolution, 279–302. Dordrecht: Springer Netherlands, 1985. http://dx.doi.org/10.1007/978-94-009-5400-7_24.
Der volle Inhalt der QuelleEmel’yanenko, V. V. „Dynamics Of Periodic Comets And Meteor Streams“. In Dynamics and Evolution of Minor Bodies with Galactic and Geological Implications, 91–110. Dordrecht: Springer Netherlands, 1992. http://dx.doi.org/10.1007/978-94-011-2743-1_7.
Der volle Inhalt der QuelleKonferenzberichte zum Thema "Comets Dynamics"
Nishio, M., M. Yoshihara, A. Nakashima und M. Sasaki. „Development of the COMETS structure (Communications and Broadcasting Engineering Test Satellite)“. In 36th Structures, Structural Dynamics and Materials Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1995. http://dx.doi.org/10.2514/6.1995-1511.
Der volle Inhalt der QuelleFinklenburg, Susanne, Nicolas Thomas, Jörg Knollenberg und Ekkehard Kührt. „Comparison of DSMC and Euler Equations Solutions for Inhomogeneous Sources on Comets“. In 27TH INTERNATIONAL SYMPOSIUM ON RAREFIED GAS DYNAMICS. AIP, 2011. http://dx.doi.org/10.1063/1.3562799.
Der volle Inhalt der QuelleHILL, STEVEN, und TODD MCCUSKER. „COMET Recovery System flight dynamics“. In Flight Simulation and Technologies. Reston, Virigina: American Institute of Aeronautics and Astronautics, 1993. http://dx.doi.org/10.2514/6.1993-3693.
Der volle Inhalt der QuelleByram, Sharyl, Daniel Scheeres und Michael Combi. „Realistic Models for the Comet Dynamical Environment“. In AIAA/AAS Astrodynamics Specialist Conference and Exhibit. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2006. http://dx.doi.org/10.2514/6.2006-6288.
Der volle Inhalt der QuelleCosta, Marc, Miguel Pérez, Miguel Almeida, Mike Ashman, Raymond Hoofs, Steve Chien, Federico Nespoli, Juan José García und Michael Kueppers. „Rosetta: rapid science operations for a dynamic comet“. In SpaceOps 2016 Conference. Reston, Virginia: American Institute of Aeronautics and Astronautics, 2016. http://dx.doi.org/10.2514/6.2016-2538.
Der volle Inhalt der Quellevan der Mark, Martin B. „Electrifying catheters by fiber optics, MRI compatibility and everything else that comes for free (Conference Presentation)“. In Dynamics and Fluctuations in Biomedical Photonics XV, herausgegeben von Valery V. Tuchin, Kirill V. Larin, Martin J. Leahy und Ruikang K. Wang. SPIE, 2018. http://dx.doi.org/10.1117/12.2302364.
Der volle Inhalt der QuelleWang, Haowei, Yicheng Pan, Meng Ma und Ping Wang. „When Dynamic Causality Comes to Graph-Temporal Neural Network“. In 2022 International Joint Conference on Neural Networks (IJCNN). IEEE, 2022. http://dx.doi.org/10.1109/ijcnn55064.2022.9892477.
Der volle Inhalt der QuelleWilliamsen, Joel, William Bohl, Jeremy Stober, Tim Flora und H. Evans. „Flying Through a Comet: Designing Structural Protection for the Deep Impact Spacecraft“. In 43rd AIAA/ASME/ASCE/AHS/ASC Structures, Structural Dynamics, and Materials Conference. Reston, Virigina: American Institute of Aeronautics and Astronautics, 2002. http://dx.doi.org/10.2514/6.2002-1608.
Der volle Inhalt der QuelleTenishev, Valeriy, Martin Rubin und Michael R. Combi. „Kinetic simulation of neutral∕ionized gas and electrically charged dust in the coma of comet 67P∕Churyumov-Gerasimenko“. In 27TH INTERNATIONAL SYMPOSIUM ON RAREFIED GAS DYNAMICS. AIP, 2011. http://dx.doi.org/10.1063/1.3562802.
Der volle Inhalt der QuelleBadescu, M., R. Bonitz, A. Ganino, N. Haddad, P. Walkemeyer, P. Backes, L. Shiraishi et al. „Dynamic acquisition and Retrieval Tool (DART) for comet sample return“. In 2013 IEEE Aerospace Conference. IEEE, 2013. http://dx.doi.org/10.1109/aero.2013.6496920.
Der volle Inhalt der QuelleBerichte der Organisationen zum Thema "Comets Dynamics"
Perdigão, Rui A. P. Earth System Dynamic Intelligence - ESDI. Meteoceanics, April 2021. http://dx.doi.org/10.46337/esdi.210414.
Der volle Inhalt der QuelleBehr, Marek, Daniel M. Pressel, Walter B. Sturek und Sr. Comments on Computational Fluid Dynamics (CFD) Code Performance on Scalable Architectures. Fort Belvoir, VA: Defense Technical Information Center, Dezember 2002. http://dx.doi.org/10.21236/ada409739.
Der volle Inhalt der QuelleFabio Morales, Leonardo, Eleonora Dávalos und Raquel Zapata. Estimating Vacancy Stocks from Aggregated Data on Hires: A Methodology to Study Frictions in the Labor Market. Banco de la República de Colombia, April 2023. http://dx.doi.org/10.32468/be.1228.
Der volle Inhalt der QuelleScollay, Robert. Asia's Infrastructure, Trade Costs and Regional Co-operation: Comments. Inter-American Development Bank, Juni 2008. http://dx.doi.org/10.18235/0006850.
Der volle Inhalt der QuelleTacsir, Ezequiel. Innovation in Services: The Hard Case for Latin America and the Caribbean. Inter-American Development Bank, November 2011. http://dx.doi.org/10.18235/0006897.
Der volle Inhalt der QuelleAjzenman, Nicolás, und Laura Jaitman. Crime Concentration and Hot Spot Dynamics in Latin America. Inter-American Development Bank, Juni 2016. http://dx.doi.org/10.18235/0011745.
Der volle Inhalt der QuelleCampbell, John, und Jianping Mei. Where do Betas Come From? Asset Price Dynamics and the Sources of Systematic Risk. Cambridge, MA: National Bureau of Economic Research, April 1993. http://dx.doi.org/10.3386/w4329.
Der volle Inhalt der QuelleAlvaredo, Facundo, François Bourguignon, Francisco H. G. Ferreira und Nora Lustig. Seventy-five Years of Measuring Income Inequality in Latin America. Inter-American Development Bank, Oktober 2023. http://dx.doi.org/10.18235/0005211.
Der volle Inhalt der QuelleChen. PR-224-03158-R01 Static and Cyclic Surface Loading on the Performance of Welds in Pre-1970 Pipelines. Chantilly, Virginia: Pipeline Research Council International, Inc. (PRCI), August 2009. http://dx.doi.org/10.55274/r0010973.
Der volle Inhalt der QuelleMuhyiddin, Muhyiddin. Indonesia Employment Report 2023. Pusat Pengembangan Kebijakan Ketenagakerjaan Kementerian Ketenagakerjaan, Dezember 2023. http://dx.doi.org/10.47198/report.2023.
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