Liberdade de associação e os desafios das organizações da sociedade civil no Brasil

O presente estudo tem por objetivo identificar de que forma o direito de liberdade de associação vem sendo aplicado com relação às organizações da sociedade civil no Brasil. A partir da análise das diferentes dimensões da liberdade de associação e das normas que tratam das organizações da sociedade civil no Brasil pós Constituição Federal de 1988, apresentamos os principais desafios a serem superados para que as organizações da sociedade civil sejam tratadas de forma a melhor garantir o direito de liberdade de associação e um marco regulatório mais adequado ao seu desenvolvimento.

Valor de marca-país: uma investigação empírica em diferentes modelos operacionais e relações com imagem de país e percepção de cultura

Atualmente, os valores intangíveis são cada vez mais importantes no processo gerencial de empresas e governos, implicando a necessidade de informações mais precisas. Dentre os ativos intangíveis mais importantes encontram-se as marcas. É por meio das marcas que os consumidores escolhem e memorizam suas compras, e assim destinam seu dinheiro para algo que possa solucionar problemas em suas vidas. Marcas são formas de empresas e países conseguirem se diferenciar no mercado competitivo globalizado, e estas últimas são denominadas marca-país. A marca-país é fonte de conhecimento e associações no mercado, e torna o país mais ou menos atraente para os estrangeiros. Para se medir o valor de uma marca-país (country brand equity) utilizamse métodos específicos. Essa métrica perceptual é uma construção de valores baseados na marca-país, como conhecimento, associações, imagem, qualidade percebida e lealdade. Este trabalho visa compor um modelo de mensuração de country brand equity aplicável à realidade brasileira. Para tanto foram apresentados diversos modelos de avaliação de marcas e marca-país, por serem complementares, e testados empiricamente. Os dois principais modelos utilizados neste trabalho foram o modelo de valor de marca de Yoo, Donthu e Lee (2000), e o modelo de valor de marca-país de Pappu e Quester (2010). Como o construto de valor de marca-país é derivado de dimensões formativas que o compõem, foram somadas nessa equação as dimensões de imagem baseada na personalidade (AAKER, 1997) e percepção de cultura (NEWMAN; NOLLEN, 1996; HOFSTEDE; BOND, 1984). Todas as variáveis e composições de dimensões foram avaliadas quanto à sua confiabilidade, linearidade, normalidade, heterocedasticidade, multicolinearidade, correlações, formação de fatores e, por fim, avaliadas em regressões e modelos de equações estruturais. Foram criados dezesseis (16) modelos iniciais, nos quais se avaliou o poder de explicação dos construtos com a variável dependente proposta por Zeugner-Roth, Diamantopoulos e Montesinos (2008). Verificou-se pouca variabilidade entre os modelos. Em seguida, foram elaborados mais oito (8) modelos com a proxy de valor de marca-país pela reputação de marca-país, proposta por Kang e Yang (2010), na qual se pôde observar que os modelos com maior número de dimensões se mostraram melhores para explicar a variável dependente. Além disso, verificou-se a importância das dimensões de imagem e percepção de cultura nesses construtos. Por fim, esta tese apresenta modelos mais consistentes de avaliação de marca-país.

An accurate distance scale to the extremely massive cluster Stephenson 2

Discoveries during the last two years have revealed the existence of a vast region of star formation close to the base of the Scutum Arm, where at least five clusters of red supergiants have been found. In order to understand the nature of this region, we need to determine accurate distances to the clusters. We present here the first results of an ongoing program to derive fundamental parameters (such as age, distance, etc.) to the massive cluster Stephenson 2 studying for the first time its main sequence stars.

The young open cluster Berkeley 55

We present UBV photometry of the highly reddened and poorly studied open cluster Berkeley 55, revealing an important population of B-type stars and several evolved stars of high luminosity. Intermediate-resolution far-red spectra of several candidate members confirm the presence of one F-type supergiant and six late supergiants or bright giants. The brightest blue stars are mid-B giants. Spectroscopic and photometric analyses indicate an age 50 ± 10 Myr. The cluster is located at a distance d ≈ 4 kpc, consistent with other tracers of the Perseus Arm in this direction. Berkeley 55 is thus a moderately young open cluster with a sizable population of candidate red (super)giant members, which can provide valuable information about the evolution of intermediate-mass stars.

An obscured cluster associated with the H II region RCW173

Context. The discovery of several clusters of red supergiants towards l = 24°−30° has triggered interest in this area of the Galactic plane, where lines of sight are very complex and previous explorations of the stellar content were very preliminary. Aims. We attempt to characterise the stellar population associated with the H ii region RCW 173 (=Sh2-60), located at, as previous studies have suggested that this population could be beyond the Sagittarius arm. Methods. We obtained UBV photometry of a stellar field to the south of the brightest part of RCW 173, as well as spectroscopy of about twenty stars in the area. We combined our new data with archival 2MASS near-infrared photometry and Spitzer/GLIMPSE imaging and photometry, to achieve a more accurate characterisation of the stellar sources and the associated cloud. Results. We find a significant population of early-type stars located at d = 3.0 kpc, in good agreement with the “near” dynamical distance to the H ii region. This population should be located at the near intersection of the Scutum-Crux arm. A luminous O7 II star is likely to be the main source of ionisation. Many stars are concentrated around the bright nebulosity, where GLIMPSE images in the mid infrared show the presence of a bubble of excited material surrounding a cavity that coincides spatially with a number of B0-1 V stars. We interpret this as an emerging cluster, perhaps triggered by the nearby O7 II star. We also find a number of B-type giants. Some of them are located at approximately the same distance, and may be part of an older population in the same area, characterised by much lower reddening. A few have shorter distance moduli and are likely to be located in the Sagittarius arm. Conclusions. The line of sight in this direction is very complex. Optically visible tracers delineate two spiral arms, but seem to be absent beyond d ≈ 3 kpc. Several H ii regions in this area suggest that the Scutum-Crux arm contains thick clouds actively forming stars. All these populations are projected on top of the major stellar complex signposted by the clusters of red supergiants.

NGC 7419 as a template for red supergiant clusters

Context. The open cluster NGC 7419 is known to contain five red supergiants and a very high number of Be stars. However, there are conflicting reports about its age and distance that prevent a useful comparison with other clusters. Aims. We intend to obtain more accurate parameters for NGC 7419, using techniques different from those of previous authors, so that it may be used as a calibrator for more obscured clusters. Methods. We obtained Strömgren photometry of the open cluster NGC 7419, as well as classification spectroscopy of ~20 stars in the area. We then applied standard analysis and classification techniques. Results. We find a distance of 4 ± 0.4 kpc and an age of 14 ± 2 Myr for NGC 7419. The main-sequence turn-off is found at spectral type B1, in excellent agreement. We identify 179 B-type members, implying that there are more than 1200 M⊙ in B stars at present. Extrapolating this to lower masses indicates an initial cluster mass of between 7000 and 10 000 M⊙, depending on the shape of the initial mass function. We find a very high fraction (≈40%) of Be stars around the turn-off, but very few Be stars at lower masses. We also report for the first time a strong variability in the emission characteristics of Be stars. We verified that the parameters of the red supergiant members can be used to obtain accurate cluster parameters. Conclusions. NGC 7419 is sufficiently massive to serve as a testbed for theoretical predictions and as a template to compare more obscured clusters. The distribution of stars above the main-sequence turn-off is difficult to accommodate with current evolutionary tracks. Though the presence of five red supergiants is marginally consistent with theoretical expectations, the high number of Be stars and very low number of luminous evolved B stars hint at some unknown physical factor that is not considered in current synthesis models.

Massive open star clusters using the VVV survey III. A young massive cluster at the far edge of the Galactic bar

Context. Young massive clusters are key to map the Milky Way’s structure, and near-infrared large area sky surveys have contributed strongly to the discovery of new obscured massive stellar clusters. Aims. We present the third article in a series of papers focused on young and massive clusters discovered in the VVV survey. This article is dedicated to the physical characterization of VVV CL086, using part of its OB-stellar population. Methods. We physically characterized the cluster using JHKS near-infrared photometry from ESO public survey VVV images, using the VVV-SkZ pipeline, and near-infrared K-band spectroscopy, following the methodology presented in the first article of the series. Results. Individual distances for two observed stars indicate that the cluster is located at the far edge of the Galactic bar. These stars, which are probable cluster members from the statistically field-star decontaminated CMD, have spectral types between O9 and B0 V. According to our analysis, this young cluster (1.0 Myr < age < 5.0 Myr) is located at a distance of 11+5-6 kpc, and we estimate a lower limit for the cluster total mass of (2.8+1.6-1.4) · 103 M⊙. It is likely that the cluster contains even earlier and more massive stars.

Gaia-ESO Survey: Analysis of pre-main sequence stellar spectra

Context. The Gaia-ESO Public Spectroscopic Survey is obtaining high-quality spectroscopy of some 100 000 Milky Way stars using the FLAMES spectrograph at the VLT, down to V = 19 mag, systematically covering all the main components of the Milky Way and providing the first homogeneous overview of the distributions of kinematics and chemical element abundances in the Galaxy. Observations of young open clusters, in particular, are giving new insights into their initial structure, kinematics, and their subsequent evolution. Aims. This paper describes the analysis of UVES and GIRAFFE spectra acquired in the fields of young clusters whose population includes pre-main sequence (PMS) stars. The analysis is applied to all stars in such fields, regardless of any prior information on membership, and provides fundamental stellar atmospheric parameters, elemental abundances, and PMS-specific parameters such as veiling, accretion, and chromospheric activity. Methods. When feasible, different methods were used to derive raw parameters (e.g. line equivalent widths) fundamental atmospheric parameters and derived parameters (e.g. abundances). To derive some of these parameters, we used methods that have been extensively used in the past and new ones developed in the context of the Gaia-ESO survey enterprise. The internal precision of these quantities was estimated by inter-comparing the results obtained by these different methods, while the accuracy was estimated by comparison with independent external data, such as effective temperature and surface gravity derived from angular diameter measurements, on a sample of benchmarks stars. A validation procedure based on these comparisons was applied to discard spurious or doubtful results and produce recommended parameters. Specific strategies were implemented to resolve problems of fast rotation, accretion signatures, chromospheric activity, and veiling. Results. The analysis carried out on spectra acquired in young cluster fields during the first 18 months of observations, up to June 2013, is presented in preparation of the first release of advanced data products. These include targets in the fields of the ρ Oph, Cha I, NGC 2264, γ Vel, and NGC 2547 clusters. Stellar parameters obtained with the higher resolution and larger wavelength coverage from UVES are reproduced with comparable accuracy and precision using the smaller wavelength range and lower resolution of the GIRAFFE setup adopted for young stars, which allows us to provide stellar parameters with confidence for the much larger GIRAFFE sample. Precisions are estimated to be ≈120 K rms in Teff, ≈0.3 dex rms in log g, and ≈0.15 dex rms in [Fe/H] for the UVES and GIRAFFE setups.

Catharine Waugh McCullouch papers in the Mary Earhart Dillon collection, 1869-1945

Collection primarily documents McCulloch's research on women's legal status, and her work with the Illinois Equal Suffrage Association, the National American Woman Suffrage Association, and the League of Women Voters. There is also documentation of women in the legal profession, of McCulloch's friendships with the other women suffragists and lawyers, and some biographical material. The papers contain little information about her family or social life.

A collection of the most approved pieces of music from various authors: transcribed while member of Harvard University, from July 1789 to July 1793

John Pierce kept this journal while he was a student at Harvard College. It consists of manuscript musical scores with annotations indicating the occasions at which the music was performed. These occasions included commencements, public exhibitions and Dudleian lectures. A note indicates that one anthem was prepared by Samuel Holyoke at Pierce's request, to be performed at Pierce's class commencement exercises, held on July 13, 1793. Several annotations were made in May 1794, the year following Pierce's graduation. There is a table of contents on the last page.

Birthplace Effects on the Development of Female Athletic Talent

This study examined the extent to which an athlete's place of birth can influence the likelihood of playing professional sport. Information regarding the birthplace of all American female athletes in the Ladies Professional Golf Association and Women's United Soccer Association was gathered from official league websites. Monte Carlo simulations were used to determine if the birthplace of these professional athletes differed in any systematic way from official census population distributions. Odds-ratios were determined for cities within specific population ranges to ascertain if the likelihood of playing professional sport was influenced in any systematic way by city size. The analyses revealed that female professional soccer players born in cities of less than 1,000,000 were over-represented, as were female professional golfers born in cities of less than 250,000. Results are consistent with those of male professional athletes in suggesting that areas of lower population provide conditions more conducive to the development of expertise than do larger city environments.

Ties That Bind? The Parapublic Underpinnings of Franco-German Relations as Construction of International Value. CES Germany & Europe Working Papers, No. 02.4, 2002

Beneath the relations among states, and distinct from the exchanges of an autonomous regional or global civil society, there is another set of international practices which is neither public nor private but parapublic. The Franco-German parapublic underpinnings consist of publicly funded youth and educational exchanges, some two thousand city and regional partnerships, a host of institutes and associations concerned with Franco-German matters, and various other parapublic elements. This institutional reality provides resources, socializes the participants of its programs, and generates social meaning. Simultaneously, parapublic activity faces severe limits. In this paper I clarify the concept of “parapublic underpinnings” of international relations and flesh out their characteristics for the relationship between France and Germany. I then evaluate the effects and limits of this type of activity, and relate this paper’s findings and arguments to recent research on transnationalism, Europeanization, and denationalization.

Women's political participation in Tunisia. Arab Citizenship Review No. 14, 21 January 2016

The collapse of the authoritarian regime in Tunisia in 2011 has given women new opportunities to participate in political life and in civil society activities, standing for elections (2011 and 2014) or becoming members of political parties and associations. Nevertheless, despite these advances and the already positive point of de- parture thanks to the legacy of Bourguiba, the “liberator of the country and the women”, participation of women remains unsatisfactory. While Tunisian women have enjoyed extended individual rights, especially compared to Arab women in general, since the country became independent in 1956, their political participation has remained controlled by the state.T he challenge of increasing the political participation of women, even in a democratic phase of the country’s political life, remains.The new electoral laws from 2011 and 2014 endorse parity and women rights, now guaranteed by the Constitution. However, the implementation of these rights is still at stake.

Why Moldova’s European integration is failing. CEPS Commentary, 3 March 2016

As anti-government demonstrations continued in Chisinau, EU foreign ministers reaffirmed their support for Moldova’s political association and economic integration with the EU in the Council conclusions of 15 February 2016. The ministers also confirmed that all 28 EU member states have ratified the Association Agreement between Moldova and the EU. Despite this progress, Moldova’s European integration project is in tatters. According to an authoritative survey commissioned by the National Democratic Institute in November 2015, only 40% Moldovans support European integration; 44% are in favour of Eurasian integration, however. [1] As Russia steps up the pressure on Moldova, these trends are worrying for the EU.

Bulletin of the scientific laboratories of Denison University.

Title varies slightly.