Feminismo na internet: o caso do coletivo marcha das vadias e sua página no facebook

This article analyzes how the Brazilian feminist movements utilize online social networks to expand their sphere of action and mobilization in society through understanding how is the activity of the collective Marcha das Vadias of Rio de Janeiro on your Facebook page and as this group is mobilized in the online environment to organize its annual march, here, specifically the 4th Marcha das Vadias of Rio de Janeiro. Through exploratory, descriptive and analytical qualitative research methodology and analysis of social networks on the Internet, it is concluded that the network generated by the topic "4th Marcha das Vadias of Rio de Janeiro" was central dynamic between a public clear feminist, but weak and little to comprehensive dialogue with society in general positions.

Transitando entre as políticas de assistência social e igualdade racial: produção e (re)produção da trama social dos negros

Pós-graduação em Serviço Social - FCHS

Transitando entre as políticas de assistência social e igualdade racial: produção e (re)produção da trama social dos negros

Pós-graduação em Serviço Social - FCHS

Ameloblastoma demographic, clinical and treatment study - analysis of 40 cases

Dental lesions represent about 1% of oral cavity tumors being ameloblastoma the most common one. It is a tumor of epithelial origin that mainly affects the jaw, and less commonly the maxilla. Its clinical presentation is that of an asymptomatic slow-growing tumor. Despite being a benign tumor, it has an invasive behavior with a high rate of recurrence if not treated properly. Objective: To describe the cases of ameloblastoma in a reference department. Methods: Retrospective analysis of 40 cases. The variables analyzed were: age, gender, ethnicity, tumor location, type of treatment, complications and recurrence. Results: The most affected gender was male - 21 cases (52.5%); with a predominance of Caucasians - 24 cases (60%). The mean age was 35.45 years; the most common location was in.the jaw - 37 cases (92.5%). Facial asymmetry was the most frequent complaint. Of the 40 cases, 33 were submitted to surgery. Of those submitted to surgery, 24 (72.72%) underwent segmental resection, with recurrence in 4 (12.12%) cases. Conclusion: Ameloblastoma may relapse when treatment is not performed with broad surgical resection of the lesion with wide safety margins.

NGC 2782: a merger remnant with young stars in its gaseous tidal tail

We have searched for young star-forming regions around the merger remnant NGC 2782. By using Galaxy Evolution Explorer far-ultraviolet and near-ultraviolet imaging and H i data we found seven ultraviolet sources, located at distances greater than 26 kpc from the centre of NGC 2782, and coinciding with its western H i tidal tail. These regions were resolved in several smaller systems when Gemini/Gemini multi-object spectrograph (GMOS) r-band images were used. We compared the observed colours to stellar population synthesis models and found that these objects have ages of similar to 1 to 11 Myr and masses ranging from 103.9 to 104.6 M circle dot. By using Gemini/GMOS spectroscopic data we confirm memberships and derive high metallicities for three of the young regions in the tail (12+log(O/H) = 8.74 +/- 0.20, 8.81 +/- 0.20 and 8.78 +/- 0.20). These metallicities are similar to the value presented by the nuclear region of NGC 2782 and also similar to the value presented for an object located close to the main body of NGC 2782. The high metallicities measured for the star-forming regions in the gaseous tidal tail of NGC 2782 could be explained if they were formed out of highly enriched gas which was once expelled from the centre of the merging galaxies when the system collided. An additional possibility is that the tail has been a nursery of a few generations of young stellar systems which ultimately polluted this medium with metals, further enriching the already pre-enriched gas ejected to the tail when the galaxies collided.

Galaxy interactions I. Major and minor mergers

Aims. We study galaxy pair samples selected from the Sloan Digital Sky Survey (SDSS-DR7) and we perform an analysis of minor and major mergers with the aim of investigating the dependence of galaxy properties on interactions. Methods. We build a galaxy pair catalog requiring r(p) < 25 kpc h(-1) and Delta V < 350 km s(-1) within redshift z < 0.1. By visual inspection of SDSS images we remove false identifications and we classify the interactions into three categories: pairs undergoing merging, M; pairs with evident tidal features, T; and non disturbed, N. We also divide the pair sample into minor and major interactions according to the luminosity ratio of the galaxy members. We study star formation activity through colors, the 4000 angstrom break, and star formation rates. Results. We find that similar to 10% of the pairs are classified as M. These systems show an excess of young stellar populations as inferred from the D-n(4000) spectral index, colors, and star formation rates of the member galaxies, an effect which we argue is directly related to the ongoing merging process. We find similar to 30% of the pairs exhibiting tidal features (T pairs) with member galaxies showing evidence of old stellar populations. This can be associated either to the disruptive effect of some tidal interactions, or to the longer time-scale of morphological disturbance with respect to the bursts of the tidal induced star formation. Regardless of the color distribution, we find a prominent blue peak in the strongest mergers, while pairs with tidal signs under a minor merger show a strong red peak. Therefore, our results show that galaxy interactions are important in driving the evolution of galaxy bimodality. By adding stellar masses and star formation rates of the two members of the pairs, we explore the global efficiency of star formation of the pairs as a whole. We find that, at a given total stellar mass, major mergers are significantly more efficient (a factor approximate to 2) in forming new stars, with respect to both minor mergers or a control sample of non-interacting galaxies. We conclude that the characteristics of the interactions and the ratio of luminosity galaxy pair members involved in a merger are important parameters in setting galaxy properties.

TRA ANTICHE PIETRE E NUOVI CAMMINI

IL TESTO SVILUPPA IL RAPPORTO TRA ANTROLOGIA CULTURALE E TURISMO, IN PARTICOLARE LA FORMAZIONE DI OPERATORI TURISTICI IN CAMBOGIA.

Dall’intervento di mediazione culturale all’attivazione di processi di mediazione interculturale nell’ottica dell’integrazione del sistema Cacciavillani Federica e Di Bella Sofia

Questo materiale è disponibile on line. Pertanto è utile per integrare le lezioni sulla mediazione culturale