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Journal articles on the topic 'Charbonnel'

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Published: 4 June 2021

Last updated: 3 February 2022

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1

Michaud, Georges, and C. R. Proffitt. "Mechanisms of Separation of Elements." International Astronomical Union Colloquium 138 (1993): 439–49. http://dx.doi.org/10.1017/s0252921100020881.

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Since the last IAU Colloquium devoted to Ap stars, die continuous development of high signal to noise observations and of computerized analysis tools have greatly increased the effectiveness of abundance anomalies as a probe of hydrodynamical processes in stars. Until the 1980s, they seemed limited to ApBp and AmFm stars where the effects are largest. More recently the abundances of Li and He have been suggested to play important diagnostic roles for hydrodynamics in both the Sun (Proffitt and Michaud 1991b, Pinsonneault et al. 1989) and Halo stars (Proffitt and Michaud 1991a, Pinsonneault et al. 1992, Vauclair 1988, Charbonnel et al. 1992, Deliyannis and Demarque 1991). The observation of a Li abundance gap in F stars of clusters has raised the question of the link between these objects and the AmFm stars (Michaud 1986, Charbonneau and Michaud 1988, 1991) or alternately with solar type stars. The observed Li abundance on die subgiant branch sheds some light on this problem (Charbonneau et al. 1989; Charbonnel and Vauclair 1992). In solar type stars, the observed Li abundance constrains the superficial turbulence that may inhibit surface He gravitational settling (Proffitt and Michaud 1991b) whose effects can be detected using solar seismology (Guzik and Cox 1992, Dziembowski et al. 1992).

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Charbonnel, Jean, Anne Dulphy, and Christine Manigand. "Entretien avec Jean Charbonnel." Histoire@Politique 17, no. 2 (2012): 179. http://dx.doi.org/10.3917/hp.017.0179.

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3

Talon, Suzanne, and Corinne Charbonnel. "Meridional Circulation, Turbulence and Lithium in Sub-Giants Originating from the Hot Side of the Dip." Symposium - International Astronomical Union 198 (2000): 516–17. http://dx.doi.org/10.1017/s0074180900167245.

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We present the impact of meridional circulation and shear turbulence on the evolution of the lithium abundance at the surface of evolved stars originating from the hot side of the Li Dip. We show that our fully consistent treatment of the same hydrodynamical processes which can account for C and N anomalies in B type stars (Talon et al. 1997) and for the shape of the hot side of the Li dip in open clusters (Talon & Charbonnel 1998) also explains Li observations in stars with Teff higher than 7000K on the main sequence as well as in their evolved counterparts (see also Charbonnel & Talon 1999).

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4

Araújo, Alberto Filipe. "Metáfora y educación. El poder de la metáfora hortícola en el pensamiento educacional de Célestin Freinet." Teoría de la Educación. Revista Interuniversitaria 26, no. 2 (December 16, 2014): 69–91. http://dx.doi.org/10.14201/teoredu20142616991.

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El presente artículo intenta entender, en la línea de Daniel Hameline y de Nanine Charbonnel, el porqué de que en educación no se pueda escapar a la presencia y a la función que la metáfora desempeña en el interior, tanto de los textos, como de los discursos educacionales y pedagógicos. En este contexto, el autor del estudio presenta y trabaja la obra educacional de Célestin Freinet (1896-1966) influenciado por los estudios sobre la metáfora de Daniel Hameline, Nanine Charbonnel y de Paul Ricœur. Esto, con el objetivo de hacer entender la pertinencia de la metáfora hortícola en el espacio educacional pedagógico. También intenta reflexionar, en la línea de Paul Ricoeur, si la metáfora, más precisamente la metáfora hortícola, nos plantea la necesidad de una apertura al símbolo, que en el caso específico de la metáfora hortícola sería al simbolismo vegetal y, por consiguiente, habría que tener en cuenta cuáles son las consecuencias pedagógicas de esa metáfora y de la metáfora en sentido amplio.

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5

Lamarque, Gwénael. "Immuable ou inclassable ? Jean Charbonnel au Parlement (1962-1978)." Parlement[s], Revue d'histoire politique HS 5, no. 3 (2009): 85. http://dx.doi.org/10.3917/parl.hs05.0085.

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6

Charbonnel, Corinne, and Nadège Lagarde. "Thermohaline mixing in stars and the long-standing 3He problem." Proceedings of the International Astronomical Union 5, S265 (August 2009): 205–8. http://dx.doi.org/10.1017/s1743921310000554.

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AbstractThermohaline mixing has been recently identified as the dominating process that governs the photospheric composition of low-mass bright giant stars (Charbonnel & Zahn 2007). Here we present the predictions of stellar models computed with the code STAREVOL taking into account this mechanism together with rotational mixing and atomic diffusion. We compare our theorical predictions with recent observations and discuss how the corresponding yields for 3He are compatible with the observed behaviour of this light element in our Galaxy.

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7

Charbonnel, Corinne, and Nadège Lagarde. "Thermohaline mixing in stars : solving the long-standing 3He problem." Proceedings of the International Astronomical Union 5, S268 (November 2009): 441–46. http://dx.doi.org/10.1017/s1743921310004606.

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AbstractThermohaline mixing has been recently identified as the dominating process that governs the photospheric composition of low-mass bright giant stars (Charbonnel & Zahn 2007a). Here we present the predictions of stellar models computed with the code STAREVOL that takes into account this mechanism together with rotational mixing and atomic diffusion. We compare our theorical predictions with recent observations and discuss how the corresponding yields for 3He are compatible with the observed behaviour of this light element in our Galaxy.

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8

Charbonnel, Corinne, Constantine P. Deliyannis, and Marc H. Pinsonneault. "Sinks of Light Elements in Stars - Part III." Symposium - International Astronomical Union 198 (2000): 87–97. http://dx.doi.org/10.1017/s0074180900166422.

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See the abstract given in Part I (Deliyannis, Pinsonneault, Charbonnel, hereafter DPC, this volume). In Part III, we first discuss the LiBeB observations in subgiant stars and the constraints they bring on the transport processes occuring on the main sequence. Evidence is then reviewed that suggests that in situ mixing occurs in evolved low mass Population I and Population II stars. Theoretical mechanisms that can create such mixing are discussed, as well as their implications for the evolution of the LiBeB and 3He.

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9

Pinsonneault, Marc H., Corinne Charbonnel, and Constantine P. Deliyannis. "Sinks of Light Elements in Stars - Part II." Symposium - International Astronomical Union 198 (2000): 74–86. http://dx.doi.org/10.1017/s0074180900166410.

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See the abstract given in Part I (Deliyannis, Pinsonneault, Charbonnel, hereafter DPC, in these proceedings). In Part II we discuss the lithium data for metal-poor stars and the constraints it places on stellar depletion. There are a variety of indicators that place interesting bounds on the degree of stellar depletion, and in contrast to the other two sections the data for Population II stars provides weaker evidence for stellar lithium depletion. We review both the theoretical studies and the observational data, and critically evaluate the degree of stellar depletion consistent with the data.

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10

Leroy, Sarah. "Nadine Charbonnel et Georges Kleiber (éd.), La métaphore entre philosophie et rhétorique." Cahiers de praxématique, no. 36 (January 1, 2001): 221–23. http://dx.doi.org/10.4000/praxematique.380.

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11

Novitsky, Anthony W. "Edmond Michelet. By Jean Charbonnel. Politiques & Chrétiens. Paris: Beauchesne, 1987. 294 pp. F 120." Church History 58, no. 2 (June 1989): 259–60. http://dx.doi.org/10.2307/3168760.

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12

Szécsi, Dorottya, Jonathan Mackey, and Norbert Langer. "Core-hydrogen-burning RSGs in the early globular clusters." Proceedings of the International Astronomical Union 11, A29B (August 2015): 473. http://dx.doi.org/10.1017/s1743921316005901.

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AbstractThe first stellar generation in galactic globular clusters contained massive low-metallicity stars (Charbonnel et al. 2014). We modelled the evolution of this massive stellar population and found that such stars with masses 100-600 M⊙ evolve into cool RSGs (Szécsi et al. 2015). These RSGs spend not only the core-He-burning phase but even the last few 105 years of the core-H-burning phase on the SG branch. Due to the presence of hot massive stars in the cluster at the same time, we show that the RSG wind is trapped into photoionization confined shells (Mackey et al. 2014). We simulated the shell formation around such RSGs and find them to become gravitationally unstable (Szécsi et al. 2016). We propose a scenario in which these shells are responsible for the formation of the second generation low-mass stars in globular clusters with anomalous surface abundances.

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Chiappini, Cristina, and Francesca Matteucci. "The Evolution of 3He, 4He and D in the Galaxy." Symposium - International Astronomical Union 198 (2000): 540–46. http://dx.doi.org/10.1017/s0074180900167294.

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In this work we present the predictions of a modified version of the ‘two-infall model’ (Chiappini et al. 1997 - CMG) for the evolution of 3He, 4He and D in the solar vicinity, as well as their distributions along the Galactic disk. In particular, we show that when allowing for extra-mixing process in low mass stars (M < 2.5 M⊙), as predicted by Charbonnel and do Nascimento (1998), a long standing problem in chemical evolution is solved, namely: the overproduction of 3He by the chemical evolution models as compared to the observed values in the sun and in the interstellar medium. Moreover, we show that chemical evolution models can constrain the primordial value of the deuterium abundance and that a value of (D/H)p < 3 × 10—5 is suggested by the present model. Finally, adopting the primordial 4He abundance suggested by Viegas et al. (1999), we obtain a value for ΔY/ΔZ ≃ 2 and a better agreement with the solar 4He abundance.

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14

Grimaldi, A. "Débat entre Bernard Charbonnel et Michel Marre : quelle place pour les sulfamides hypoglycémiants dans le traitement du diabète de type 2 ?" Médecine des Maladies Métaboliques 11, no. 6 (October 2017): 537–38. http://dx.doi.org/10.1016/s1957-2557(17)30124-4.

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15

Vandeloise, Claude. "La métaphore : entre philosophie et rhétorique. Nadine Charbonnel, Georges Kleiber et coll., Paris, Presses Universitaires de France, 1999, 245 pages, 198 FF." Revue québécoise de linguistique 29, no. 2 (2001): 123. http://dx.doi.org/10.7202/039445ar.

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16

Konstantinova-Antova, Renada, Michel Aurière, Corinne Charbonnel, Natalia Drake, Gregg Wade, Svetla Tsvetkova, Pascal Petit, Klaus-Peter Schröder, and Agnes Lèbre. "Magnetic fields in single late-type giants in the Solar vicinity: How common is magnetic activity on the giant branches?" Proceedings of the International Astronomical Union 9, S302 (August 2013): 373–76. http://dx.doi.org/10.1017/s174392131400252x.

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AbstractWe present our first results on a new sample containing all single G, K and M giants down to V = 4 mag in the Solar vicinity, suitable for spectropolarimetric (Stokes V) observations with Narval at TBL, France. For detection and measurement of the magnetic field (MF), the Least Squares Deconvolution (LSD) method was applied (Donati et al. 1997) that in the present case enables detection of large-scale MFs even weaker than the solar one (the typical precision of our longitudinal MF measurements is 0.1-0.2 G). The evolutionary status of the stars is determined on the basis of the evolutionary models with rotation (Lagarde et al. 2012; Charbonnel et al., in prep.) and fundamental parameters given by Massarotti et al. (1998). The stars appear to be in the mass range 1-4 M⊙, situated at different evolutionary stages after the Main Sequence (MS), up to the Asymptotic Giant Branch (AGB).The sample contains 45 stars. Up to now, 29 stars are observed (that is about 64% of the sample), each observed at least twice. For 2 stars in the Hertzsprung gap, one is definitely Zeeman detected. Only 5 G and K giants, situated mainly at the base of the Red Giant Branch (RGB) and in the He-burning phase are detected. Surprisingly, a lot of stars ascending towards the RGB tip and in early AGB phase are detected (8 of 13 observed stars). For all Zeeman detected stars v sin i is redetermined and appears in the interval 2-3 km/s, but few giants with MF possess larger v sin i.

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17

Giroux, Aline. "Charbonnel, N. (1991, 1993). La tâche aveugle (Volume 1 — Les aventures de la métaphore; Volume 2 — L’important c’est d’être propre; Volume 3 — Philosophie du modèle). Strasbourg : Presses universitaires de Strasbourg." Revue des sciences de l'éducation 22, no. 1 (1996): 186. http://dx.doi.org/10.7202/031859ar.

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18

Limongi, Marco, John C. Lattanzio, Corinne Charbonnel, Inma Dominguez, Jordi Isern, Amanda Karakas, Claus Leitherer, Marcella Marconi, Giora Shaviv, and Jacco van Loon. "DIVISION G COMMISSION 35: STELLAR CONSTITUTION." Proceedings of the International Astronomical Union 11, T29A (August 2015): 436–52. http://dx.doi.org/10.1017/s1743921316000909.

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Commission 35 (C35), “Stellar Constitution”, consists of members of the International Astronomical Union whose research spans many aspects of theoretical and observational stellar physics and it is mainly focused on the comprehension of the properties of stars, stellar populations and galaxies. The number of members of C35 increased progressively over the last ten years and currently C35 comprises about 400 members. C35 was part of Division IV (Stars) until 2014 and then became part of Division G (Stars and Stellar Physics), after the main IAU reorganisation in 2015. Four Working Groups have been created over the years under Division IV, initially, and Division G later: WG on Active B Stars, WG on Massive Stars, WG on Abundances in Red Giant and WG on Chemically Peculiar and Related Stars. In the last decade the Commission had 4 presidents, Wojciech Dziembowski (2003-2006), Francesca D'Antona (2006-2009), Corinne Charbonnel (2009-2012) and Marco Limongi (2012-2015), who were assisted by an Organizing Committee (OC), usually composed of about 10 members, all of them elected by the C35 members and holding their positions for three years. The C35 webpage (http://iau-c35.stsci.edu) has been designed and continuously maintained by Claus Leitherer from the Space Telescope Institute, who deserves our special thanks. In addition to the various general information on the Commission structure and activities, it contains links to various resources, of interest for the members, such as stellar models, evolutionary tracks and isochrones, synthetic stellar populations, stellar yields and input physics (equation of state, nuclear cross sections, opacity tables), provided by various groups. The main activity of the C35 OC is that of evaluating, ranking and eventually supporting the proposals for IAU sponsored meetings. In the last decade the Commission has supported several meetings focused on topics more or less relevant to C35. Since the primary aim of this document is to present the main activity of C35 over the last ten years, in the following we present some scientific highlights that emerged from the most relevant IAU Symposia and meetings supported and organized by C35 in the last decade.

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19

Santos, Bárbara Da Silva, and Evelyn De Almeida Orlando. "Religião, educação e política na trajetória intelectual do padre Paul-Eugène Charbonneau / Religion, education and politics in the intellectual trajectory of priest Paul-Eugène Charbonneau." Revista de História e Historiografia da Educação 3, no. 8 (August 30, 2019): 135. http://dx.doi.org/10.5380/rhhe.v3i8.67450.

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Este artigo aborda aspectos da trajetória do padre canadense Paul-Eugène Charbonneau, que atuou no Brasil, a partir de diferentes campos, intervindo na configuração da sociedade brasileira por meio da educação e da cultura. Com base na produção escrita deste intelectual, buscamos, neste artigo, apontar como a religião, a política e a educação estiveram presentes na trajetória intelectual do padre Charbonneau. Os conceitos de intelectual e elites culturais de Sirinelli (1998; 2003) e de trajetória, capital social, capital cultural e de campo de Bourdieu (2000; 2003; 2004; 2007) embasaram o aporte teórico do texto. Pensar a trajetória do intelectual Charbonneau permeada pelos campos da religião, educação e política, é perceber que a sua produção escrita não estava associada apenas à disseminação dos saberes educacionais com princípios católicos, mas trouxe discussões sobre o contexto político da época, ora trazendo elementos cristãos, ora incorporando o ator do político e cidadão brasileiro que se tornou.***This article approaches trajectory aspects of Canadian priest Paul-Eugène Charbonneau, who worked in Brazil, from different fields, intervening in the configuration of Brazilian society through education and culture. Based on the written production of this intellectual, we seek to point out how religion, politics and education were present in the intellectual trajectory of Father Charbonneau. Concepts like intellectual and cultural elites, by Sirinelli (1998, 2003), and Bourdieu's trajectory, social capital, cultural capital and field (2000, 2003, 2004, 2007) were the theoretical basis of this text. To think about the trajectory of intellectual Charbonneau, permeated by the fields of religion, education and politics, is to realize that his written production was not only associated with the dissemination of educational knowledge with Catholic principles, but brought discussions about the political context of the time, sometimes bringing Christian elements, sometimes incorporating the actor of the politician and Brazilian citizen hia had become.

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20

de Montalembert, Marc. "Hommage à Pierre Charbonneau." Vie sociale 4, no. 4 (2011): 7. http://dx.doi.org/10.3917/vsoc.114.0007.

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21

Baldi, Caterina, Sauro Lorenzini, and Enrico Selvi. "Un liquide synovial charbonneux." Revue du Rhumatisme 80, no. 5 (October 2013): 524. http://dx.doi.org/10.1016/j.rhum.2013.03.001.

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22

GODARD, O. "Réponse à Simon Charbonneau." Nature Sciences Sociétés 8, no. 4 (October 2000): 54–56. http://dx.doi.org/10.1016/s1240-1307(01)80007-8.

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23

Godard, Olivier. "Réponse à Simon Charbonneau." Natures Sciences Sociétés 8, no. 4 (October 2000): 54–56. http://dx.doi.org/10.1051/nss/20000804054.

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24

McConville, Adam. "Verify by Joelle Charbonneau." Bulletin of the Center for Children's Books 73, no. 1 (2019): 12–13. http://dx.doi.org/10.1353/bcc.2019.0557.

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25

Rognon, Frédéric. "Bernard Charbonneau et Jacques Ellul." Ecologie & politique N° 44, no. 1 (2012): 67. http://dx.doi.org/10.3917/ecopo.044.0067.

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26

Spisak, April. "Dividing Eden by Joelle Charbonneau." Bulletin of the Center for Children's Books 70, no. 9 (2017): 404. http://dx.doi.org/10.1353/bcc.2017.0341.

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27

Coats, Karen. "Time Bomb by Joelle Charbonneau." Bulletin of the Center for Children's Books 71, no. 7 (2018): 284. http://dx.doi.org/10.1353/bcc.2018.0165.

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Spisak, April. "Crazy House by James Patterson and Gabrielle Charbonnet." Bulletin of the Center for Children's Books 70, no. 8 (2017): 376. http://dx.doi.org/10.1353/bcc.2017.0296.

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29

Mothu, Alain. "Vicissitudes de la « foi du charbonnier »." Littératures classiques N° 93, no. 2 (2017): 51. http://dx.doi.org/10.3917/licla1.093.0051.

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30

Massé, Bastien. "Pierre Charbonnier : d’un livre à l’autre." Archives de Philosophie Tome 84, no. 2 (May 3, 2021): 171–76. http://dx.doi.org/10.3917/aphi.842.0171.

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31

Dalix, Ky-Anne. "Jean-Pierre Charbonneau, l’urbanisme en pratique." Tous urbains N° 32, no. 4 (May 11, 2021): 48–50. http://dx.doi.org/10.3917/tu.032.0048.

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32

Robillard, Denise. "Immigration, logement, action catholique et syndicale au temps de Mgr Charbonneau (1940-1950) : son implication sociale relue à travers les réseaux sociaux." Articles 79, no. 1 (March 18, 2013): 59–70. http://dx.doi.org/10.7202/1014854ar.

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Dès son arrivée à Montréal, la situation de l’immigration créée à la faveur de la guerre donne à Mgr Charbonneau l’occasion de traduire ses convictions sociales et son ouverture d’esprit dans les domaines du logement, de l’action catholique et syndicale. Son attitude pragmatique est différente de celle, plus idéologique, des nationalistes traditionnels. Il est d’abord question de l’évolution du regard porté sur l’immigration depuis la crise de 1929. Cette évolution est prise en cause par Mgr Charbonneau de concert avec les mouvements d’action catholique, qui retiennent les aspects humains et concrets du logement. Quant à l’action catholique, une véritable lutte de pouvoir se livre entre les mouvements spécialisés favorisés par l’archevêque dans sa lettre de 1941, et les associations comme l’Association catholique de la jeunesse canadienne (ACJC), à saveur nationaliste, dirigées par les jésuites depuis le début du XXe siècle.

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33

Segata, Jean. "DESCOLA, Philippe. La composition des mondes: entretiens avec Pierre Charbonnier. Paris: Flammarion, 2014. 381 p." Ilha Revista de Antropologia 17, no. 2 (December 27, 2015): 149. http://dx.doi.org/10.5007/ilha.v17i2.42468.

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<p>http://dx.doi.org/10.5007/2175-8034.2015v17n2p149</p><p>Philippe Descola tem sido apontado como um dos mais importantes antropólogos dos últimos anos. De suas pesquisas resultou o aparecimento de diversos trabalhos que se dispõem à discussão, à evidência ou à apresentação de sua obra. Esse é o caso de La composition des mondes, fruto de entrevistas com o jovem filósofo Pierre Charbonnier, chargé de recherche no Institut Marcel Mauss da École des Hautes Études en Sciences Sociales (EHESS). Charbonnier tem se dedicado ao estudo das noções de natureza, ecologia e ambiente na antropologia, o que faz da obra de Philippe Descola uma de suas interlocuções privilegiadas, como aquela que acontece em seu outro recente trabalho, intitulado La fin d’un grand partage: nature et société, de Durkheim à Descola (publicado em 2015, pela CNRS Édition – Paris).</p>

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Segata, Jean. "DESCOLA, Philippe. La composition des mondes: entretiens avec Pierre Charbonnier. Paris: Flammarion, 2014. 381 p." Ilha Revista de Antropologia 17, no. 2 (December 27, 2015): 149. http://dx.doi.org/10.5007/2175-8034.2015v17n2p149.

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<p>http://dx.doi.org/10.5007/2175-8034.2015v17n2p149</p><p>Philippe Descola tem sido apontado como um dos mais importantes antropólogos dos últimos anos. De suas pesquisas resultou o aparecimento de diversos trabalhos que se dispõem à discussão, à evidência ou à apresentação de sua obra. Esse é o caso de La composition des mondes, fruto de entrevistas com o jovem filósofo Pierre Charbonnier, chargé de recherche no Institut Marcel Mauss da École des Hautes Études en Sciences Sociales (EHESS). Charbonnier tem se dedicado ao estudo das noções de natureza, ecologia e ambiente na antropologia, o que faz da obra de Philippe Descola uma de suas interlocuções privilegiadas, como aquela que acontece em seu outro recente trabalho, intitulado La fin d’un grand partage: nature et société, de Durkheim à Descola (publicado em 2015, pela CNRS Édition – Paris).</p>

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35

Agar, Michael. ": Rate It X . Lynn Campbell, Claudette Charbonneau." American Anthropologist 90, no. 4 (December 1988): 1043–44. http://dx.doi.org/10.1525/aa.1988.90.4.02a00980.

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36

Potter, Polyxeni. "Experimentation du virus charbonneux: "Le Pelerin," 1922." Emerging Infectious Diseases 8, no. 2 (February 2002): 231. http://dx.doi.org/10.3201/eid0802.020200.

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37

Poirier, Roger. "Engagement social du diocèse Gatineau-Hull (1963-1987)." Les pratiques sociales d’hier 8, no. 1 (January 22, 2008): 173–83. http://dx.doi.org/10.7202/301312ar.

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Résumé Dans cet article, l'auteur témoigne, en le replaçant dans leur contexte ecclésial et social, de l'engagement social et pastoral de deux évêques du diocèse de Gatineau-Hull avec lesquels il a collaboré étroitement. Ces deux évêques sont Mgr Paul-Emile Charbonneau (1968-1974) et Mgr Adolphe Proulx (1974-1987).

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38

Robillard, Denise. "Pourquoi M Joseph Charbonneau a-t-il démissionné ?" Bulletin d'histoire politique 23, no. 2 (2015): 204. http://dx.doi.org/10.7202/1028893ar.

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39

Clark, John. "Bernard Charbonneau: Regionalism and the Politics of Experience." Capitalism Nature Socialism 13, no. 3 (September 2002): 41–48. http://dx.doi.org/10.1080/10455750208565487.

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40

Sanjuán, Miguel A. F. "Natural complexity: a modelling handbook by P. Charbonneau." Contemporary Physics 59, no. 2 (March 16, 2018): 214. http://dx.doi.org/10.1080/00107514.2018.1448446.

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41

Rovaletti, María Lucrecia, and Martín Pallares. "La acedia como forma de malestar en la sociedad actual." Revista Latinoamericana de Psicopatologia Fundamental 17, no. 1 (March 2014): 51–68. http://dx.doi.org/10.1590/s1415-47142014000100005.

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Partiendo de la propuesta de Theunissen, se busca realizar un regreso arqueológico respecto al concepto de melancolía en la antigüedad y de acedia medieval. Con ello, se intenta reflexionar esa trama de fatiga, aburrimiento, tedio, tristeza que se entreteje en la cultura actual. Charbonneau y Legrand (2003) designan como paradepresiones a este conjunto de problemas a menudo infrasintomáticos, demasiado lábiles y poco significativos para ser denominados síntomas.

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42

Roberge, René-Michel. "CHARBONNEAU, Paul-Eugène, L’homme à la découverte de Dieu." Laval théologique et philosophique 41, no. 2 (1985): 271. http://dx.doi.org/10.7202/400181ar.

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43

Maiseli, Baraka J., Qiang Liu, Ogada A. Elisha, and Huijun Gao. "Adaptive Charbonnier superresolution method with robust edge preservation capabilities." Journal of Electronic Imaging 22, no. 4 (December 16, 2013): 043027. http://dx.doi.org/10.1117/1.jei.22.4.043027.

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44

Andía, Juan Javier Rivera. "Descola, Philippe: La composition des mondes. Entretien avec Pierre Charbonnier." Anthropos 111, no. 1 (2016): 247–48. http://dx.doi.org/10.5771/0257-9774-2016-1-247.

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45

Verschueren, Nicolas. "L'expression culturelle de la protestation dans un ancien bassin charbonnier." Mouvements 65, no. 1 (2011): 67. http://dx.doi.org/10.3917/mouv.065.0067.

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46

Prades, J. "Bernard Charbonneau: une vie entière à dénoncer la grande imposture." Nature Sciences Sociétés 5, no. 3 (July 9, 1997): 82. http://dx.doi.org/10.1016/s1240-1307(97)81545-2.

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47

Gajera, Binit Vasant, Siddhant Raj Kapil, Dorsa Ziaei, Jayalakshmi Mangalagiri, Eliot Siegel, and David Chapman. "CT-Scan Denoising Using a Charbonnier Loss Generative Adversarial Network." IEEE Access 9 (2021): 84093–109. http://dx.doi.org/10.1109/access.2021.3087424.

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48

Schaffner, Martin. "Pierre Charbonnier La fin d’un grand partage. Nature et société de Durkheim à Descola Philippe Descola La composition des mondes. Entretiens avec Pierre Charbonnier." Historische Anthropologie 25, no. 2 (October 26, 2017): 286–87. http://dx.doi.org/10.7788/ha-2017-0209.

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49

Dumas1, Alexandre. "« Les évêques mangent dans ma main » : les relations entre l’Église et l’État sous Maurice Duplessis (1944-1959)." Revue d’histoire de l’Amérique française 69, no. 4 (June 2, 2016): 47–69. http://dx.doi.org/10.7202/1036514ar.

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L’historiographie, comme la mémoire populaire québécoise, entretient l’image d’une entente cordiale entre l’Église et l’Union nationale de Maurice Duplessis à laquelle la figure controversée de Mgr Joseph Charbonneau serait la seule exception. Les travaux des historiens se sont malheureusement souvent limités à une relecture des recherches déjà effectuées par Robert Rumilly et Conrad Black, dont le biais idéologique a pourtant été critiqué. Les archives religieuses, qui s’ouvrent progressivement aux chercheurs, permettent d’élaborer une vision plus complète et nuancée des rapports entre le gouvernement provincial et l’épiscopat.

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50

Y, Li, and P. R. Wilson. "The Internal Rotation Rate Inferred from Lowl and Gong Data: Using a Forward Method." Symposium - International Astronomical Union 185 (1998): 181–82. http://dx.doi.org/10.1017/s0074180900238588.

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Recently the LOWL Group has made available 2-year averages of frequency splitting data obtained mainly for low values of the degree ℓ. Charbonneau et al. (1997) find a nearly flat rotational curve in the deep radiative core from these data using a Genetic Forward Modeling method. Subsequently, they test the assumption of latitude independence for r < 0.5 by performing a 1.5-D inversion, and find a rotation rate which is 25% greater at the pole than at the equator for 0.1 < r < 0.2.

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