Dumas, Montépin e du Terrail: a circulação dos romances-folhetins franceses no Pará nos anos de 1871 a 1880

Esta dissertação tem por objetivo compreender a natureza da circulação dos romances-folhetins de autores franceses no jornal paraense intitulado O Liberal do Pará, no período de 1871 a 1880 do século XIX. Dentre os autores franceses que publicaram seus romances-folhetins nesse jornal, destacamos Alexandre Dumas pai, Ponson du Terrail e Xavier de Montépin. Além disso, busca demonstrar a dinâmica de circulação dos romances-folhetins intitulados Blanche de Beaulieu (Alexandre Dumas), A Fada D’Auteuil (Ponson du Terrail) e O Médico dos Pobres (Xavier de Montépin) no jornal O Liberal do Pará, durante um período ímpar na cidade de Belém – o momento da Belle Époque paraense, onde foram registradas inúmeras transformações no campo cultural, econômico e urbanístico do Pará oitocentista. Por fim, propõe uma análise de tais prosas de ficção, destacando as suas estruturas, as personagens e as temáticas como elementos modeladores de costumes e hábitos europeus, particularmente os de origem franceses, na província do Pará.

Um toque de voyeurismo: o diário íntimo de Couto de Magalhães (1880-1887)

O trabalho procura analisar o diário íntimo de José Vieira Couto de Magalhães, destacado político e intelectual do Brasil da segunda metade do século XIX, como registro etnográfico que ao mesmo tempo informa sobre questões prementes daquela época e evidencia o esforço de um indivíduo específico no sentido de conferir a si próprio um pouco de consistência, muito embora o diário esteja repleto de sinais de incompletude. A partir da noção do diário íntimo como prática cultural de constituição de si mesmo, faz-se uma discussão a respeito do efeito de verdade presente nesse tipo de escrita e as implicações para uso da fonte nas Ciências Sociais. Discute-se os temas mais evidentes ao longo do registro íntimo do autor: corpo, saúde e doença. Ao escrever sobre si mesmo, Couto de Magalhães evidencia o processo de educação das necessidades e das atividades corporais em muitos homens à época e, como ele dialogava com o ideal de família burguesa e higiênica que marcou o século XIX, registra a leitura de temas como homossexualismo, sonhos, casamento e medicina. O diário mostra ainda a preocupação do autor em encontrar equilíbrio entre corpo e mente, que lhe permitisse alcançar seu ideal de moderação, além do esforço em construir e legar ao futuro uma determinada imagem de si próprio.

Eletrificação, urbanização e crescimento industrial no Estado de São Paulo: 1880-1940

Pós-graduação em Geografia - IGCE

Eletrificação e crescimento industrial no estado de São Paulo: 1880-1940

O objetivo deste trabalho é evidenciar a existência de relações entre progresso técnico e desenvolvimento econômico no processo de formação da economia brasileira. Em seu aspecto mais específico, refere-se ao estudo do desenvolvimento da eletrificação e seus efeitos sobre o crescimento industrial no Estado de São Paulo, no período compreendido entre as duas décadas finais do século passado até a década de 1930. Durante este período - quando a economia e a sociedade brasileiras se transformam pelo desenvolvimento de relações de produção de natureza capitalista, ocorridas a partir do fim do escravismo, da introdução do trabalho assalariado, da expansão cafeeira, do aparecimento da ferrovia e dos bancos, das primeiras indústrias e, enfim, de atividades voltadas ao desenvolvimento do mercado interno - , o desenvolvimento da eletrificação e, especialmente, o uso de força motriz elétrica na indústria constituíram transformações essenciais. A o provocarem alterações irrevogáveis na base técnica da indústria contribuíram, também, para a alteração do padrão de acumulação.

Carlos Octavio Bunge e José Ingenieros: entre o científico e o político: pensamento racial e identidade nacional na Argentina (1880-1920)

Pós-graduação em História - FCLAS

As experiências de República no município de Franca (1880-1906)

Pós-graduação em História - FCHS

Formação de professores para o ensino inicial da leitura e da escrita, na década de 1880, em São Paulo-Brasil

Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP)

Poéticas interditas: erotismo, subversão e repúdio em Florbela Espanca (1894-1930) e Judith Teixeira (1880-1959)

Pós-graduação em Letras - FCLAS

Strategies and results of the oral cancer prevention campaign among the elderly in Sao Paulo, Brazil, 2001 to 2009

Objective. To describe the strategies and results obtained by the early diagnosis and prevention of an oral cancer campaign targeting the population aged 60 years or older developed since 2001 in the state of Sao Paulo. Methods. The main strategies used to develop the campaign were described based on the review of documents issued by the Health Ministry, National Cancer Institute, Sao Paulo State Health Department, Oncocentro Foundation of Sao Paulo, Sao Paulo City Health Department, School of Public Health at the University of Sao Paulo (USP), and Santa Marcelina Health Care Center. The impact of the campaign on the incidence of new cases of oral cancer in the target population was evaluated. Results. In 2001, 90 886 elderly were examined vs. 629 613 in 2009. The following strategies were identified: training of professionals, development of printed materials to guide municipal governments in developing the campaign and using standardized codes and criteria, guidelines for data consolidation, establishment of patient referral flows, practical training with a specialist at the basic health care unit after the follow-up examination of individuals presenting changes in soft tissues, and increase in the number of oral diagnosis services. Between 2005 and 2009, there was a significant reduction in the rate of confirmed cases of oral cancer per 100 000 individuals examined, from 20.89 to 11.12 (P = 0.00003). Conclusions. The campaign was beneficial to the oral health of the elderly and could be extended to include other age groups and regions of the country. It may also provide a basis for the development of oral cancer prevention actions in other countries, as long as local characteristics are taken into account.

THE GEMINI NICI PLANET-FINDING CAMPAIGN: DISCOVERY OF A MULTIPLE SYSTEM ORBITING THE YOUNG A STAR HD 1160

We report the discovery of two low-mass companions to the young A0V star HD 1160 at projected separations of 81 +/- 5 AU (HD 1160 B) and 533 +/- 25 AU (HD 1160 C) by the Gemini NICI Planet-Finding Campaign. Very Large Telescope images of the system taken over a decade for the purpose of using HD 1160 A as a photometric calibrator confirm that both companions are physically associated. By comparing the system to members of young moving groups and open clusters with well-established ages, we estimate an age of 50(-40)(+50) Myr for HD 1160 ABC. While the UVW motion of the system does not match any known moving group, the small magnitude of the space velocity is consistent with youth. Near-IR spectroscopy shows HD 1160 C to be an M3.5 +/- 0.5 star with an estimated mass of 0.22(-0.04)(+0.03) M-circle dot, while NIR photometry of HD 1160 B suggests a brown dwarf with a mass of 33(-9)(+12) M-Jup. The very small mass ratio (0.014) between the A and B components of the system is rare for A star binaries, and would represent a planetary-mass companion were HD 1160 A to be slightly less massive than the Sun.

The Gemini planet-finding campaign: the frequency of giant planets aroud debris disk stars

We have completed a high-contrast direct imaging survey for giant planets around 57 debris disk stars as part of the Gemini NICI Planet-Finding Campaign. We achieved median H-band contrasts of 12.4 mag at 0.''5 and 14.1 mag at 1'' separation. Follow-up observations of the 66 candidates with projected separation <500 AU show that all of them are background objects. To establish statistical constraints on the underlying giant planet population based on our imaging data, we have developed a new Bayesian formalism that incorporates (1) non-detections, (2) single-epoch candidates, (3) astrometric and (4) photometric information, and (5) the possibility of multiple planets per star to constrain the planet population. Our formalism allows us to include in our analysis the previously known β Pictoris and the HR 8799 planets. Our results show at 95% confidence that <13% of debris disk stars have a ≥5 M Jup planet beyond 80 AU, and <21% of debris disk stars have a ≥3 M Jup planet outside of 40 AU, based on hot-start evolutionary models. We model the population of directly imaged planets as d 2 N/dMdavpropm α a β, where m is planet mass and a is orbital semi-major axis (with a maximum value of a max). We find that β < –0.8 and/or α > 1.7. Likewise, we find that β < –0.8 and/or a max < 200 AU. For the case where the planet frequency rises sharply with mass (α > 1.7), this occurs because all the planets detected to date have masses above 5 M Jup, but planets of lower mass could easily have been detected by our search. If we ignore the β Pic and HR 8799 planets (should they belong to a rare and distinct group), we find that <20% of debris disk stars have a ≥3 M Jup planet beyond 10 AU, and β < –0.8 and/or α < –1.5. Likewise, β < –0.8 and/or a max < 125 AU. Our Bayesian constraints are not strong enough to reveal any dependence of the planet frequency on stellar host mass. Studies of transition disks have suggested that about 20% of stars are undergoing planet formation; our non-detections at large separations show that planets with orbital separation >40 AU and planet masses >3 M Jup do not carve the central holes in these disks.

The Gemini NICI planet-finding campaign: the frequency of giant planets around young B and A stars

We have carried out high contrast imaging of 70 young, nearby B and A stars to search for brown dwarf and planetary companions as part of the Gemini NICI Planet-Finding Campaign. Our survey represents the largest, deepest survey for planets around high-mass stars (≈1.5-2.5 M ☉) conducted to date and includes the planet hosts β Pic and Fomalhaut. We obtained follow-up astrometry of all candidate companions within 400 AU projected separation for stars in uncrowded fields and identified new low-mass companions to HD 1160 and HIP 79797. We have found that the previously known young brown dwarf companion to HIP 79797 is itself a tight (3 AU) binary, composed of brown dwarfs with masses 58$^{+21}_{-20}$ M Jup and 55$^{+20}_{-19}$ M Jup, making this system one of the rare substellar binaries in orbit around a star. Considering the contrast limits of our NICI data and the fact that we did not detect any planets, we use high-fidelity Monte Carlo simulations to show that fewer than 20% of 2 M ☉ stars can have giant planets greater than 4 M Jup between 59 and 460 AU at 95% confidence, and fewer than 10% of these stars can have a planet more massive than 10 M Jup between 38 and 650 AU. Overall, we find that large-separation giant planets are not common around B and A stars: fewer than 10% of B and A stars can have an analog to the HR 8799 b (7 M Jup, 68 AU) planet at 95% confidence. We also describe a new Bayesian technique for determining the ages of field B and A stars from photometry and theoretical isochrones. Our method produces more plausible ages for high-mass stars than previous age-dating techniques, which tend to underestimate stellar ages and their uncertainties.