Early memories of warmth and safeness and eating psychopathology: The mediating role of social safeness and body appreciation

Research on human development and functioning has highlighted the importance of early emotional and relational experiences. Particularly, an association between the absence of early positive memories and the presence of disordered eating has been evidenced by recent investigations. However, the mechanisms underlying this association remain unclear. Using a sample of 490 women, the hypothesis that early positive memories are negatively associated with disordered eating via social safeness and a positive relationship with one’s body image was tested via path analysis. The tested model explained 51% of eating psychopathology’s variance, and revealed a good adjustment to the empirical data. Additionally, social safeness and body appreciation were revealed as mediators of the impact of early warm and safe memories on disordered eating, when controlling for the effect of BMI. These findings suggest the importance of targeting social safeness and acceptance, especially when defining potentially effective programmes for the prevention of eating disorders

Experiential avoidance versus Decentering abilities: The role of different emotional processes on disordered eating

In modern Western societies, the female body is a predominantly used dimension in self and social evaluations. In fact, the perceived discrepancy between one´s current and ideal body image may act as a pathogenic phenomenon for women´s well-being. Furthermore, significant differences in the tendency to engage in disordered eating attitudes and behaviours have been verified between women sharing similar characteristics and perceptions about weight and body shape, which suggests that different emotion regulation processes may be involved in this association. This study thus aims to clarify the mediational effect of two different emotional regulation processes, experiential avoidance and decentering, on the association of weight and body shape variables and shame with disordered eating, in a sample of 760 women. The tested path model explained 44% of disordered eating attitudes and behaviours and showed an excellent model fit. Results demonstrated that Body Mass Index had a direct effect, albeit weak, on disordered eating behaviours and that body image discrepancy and shame presented indirect effects through the mechanisms of experiential avoidance and decentering. Results also revealed that experiential avoidance and decentering showed significant mediator effects on the relationship of weight and body shape and shame with disordered eating behaviors. These findings suggested that while experiential avoidance exacerbates the impact of weight and body shape and shame on disordered eating attitudes and behaviors, decentering seems to attenuate this association. Our findings appear to offer significant clinical and research implications, highlighting the importance of targeting maladaptive emotion processes through the development of decentering abilities

VARIAÇÃO ESPACIAL DO INTEMPERISMO COMO SUBSÍDIO AO ESTUDO DA DENUDAÇÃO NO MÉDIO VALE DO RIO PARAÍBA DO SUL – RJ

A variação de formas encontradas no médio vale do rio Paraíba do Sul indicam variabilidade quanto à natureza e intensidade dos processos de denudação. Busca-se explicar estas diferenças a partir da investigação granulométrica e química dos produtos de intemperismo. Os resultados apontam que os processos mecânicos são mais atuantes na sub-bacia do rio Pedras, sendo comparável a bacia do rio Bananal, enquanto que na sub-bacia do rio Turvo os processos químicos são dominantes em sua evolução

Continuous infusion of propofol after ketamine-midazolam premedication in cats

Estudaram-se os efeitos anestésicos e cardiorrespiratórios produzidos pela infusão contínua de propofol em gatos pré-medicados com a associação cetamina-midazolam. Catorze gatos adultos foram igualmente distribuídos em dois grupos (TX1 e TX3) aos quais administraram-se, pela via intramuscular, cetamina (3,0mg/kg) e midazolam (0,3mg/kg). Decorridos cinco minutos procedeu-se a indução anestésica pela administração intravenosa de propofol (5,0mg/kg), imediatamente seguida pela infusão contínua do agente hipnótico nas doses de 0,1 ou 0,3mg/kg/min, aos animais de TX1 e TX3, respectivamente. Foram mensuradas as freqüências cardíaca e respiratória, temperatura retal, saturação de oxihemoglobina, concentração exalada de dióxido de carbono e pressão arterial. Em TX3 observou-se manutenção de adequado plano anestésico, enquanto que os animais do TX1 apresentaram-se sedados. Houve decréscimo acentuado da freqüência cardíaca, pressão arterial e elevação da concentração de dióxido de carbono exalado no TX3. Conclui-se que o emprego de propofol na dose de infusão de 0,3mg/kg/min em gatos pré-medicados com cetamina-midazolam produz anestesia satisfatória, bradicardia, depressão da função respiratória e pressão arterial.Anesthetic and cardiorespiratory effects of two different infusion rates of propofol were studied in cats premedicated with ketamine-midazolam. Fourteen cats were assigned to one of the two groups (TX1 or TX3). Ketamine (3.0mg/kg) and midazolam (0.3mg/kg) were administered intramuscularly. After 5 minutes, anesthesia was induced by propofol (5.0mg/kg) and maintained by a continuous infusion of propofol (0.1 and 0.3mg/kg/min, TX1 and TX3, respectively). Heart and respiratory rate, rectal temperature, oxygen hemoglobin saturation, end-tidal carbon dioxide and arterial pressure were recorded. Adequate anesthesia was observed in TX3, while animals in TX1 were only lightly sedated. A greater decrease in heart rate, arterial pressure and elevation of end-tidal dioxide carbon was observed in TX3 compared to TX1. It was concluded that administration of propofol at infusion rate of 0.3mg/kg/min provides satisfatory anesthesia, but it results in bradycardia, depression of respiratory function and arterial pressure

The Temporal Pattern of Mating Behavior of the Fruit Fly, Anastrepha zenildae in the Laboratory

The state of Rio Grande do Norte is an important fruit-producing and exporting area in northeastern Brazil. The success of this industry depends on fruit fly population control, especially in fly-free exporting zones. However, many fruits are not exported because of quarantine restrictions imposed by importing countries. A survey in the state has detected a considerable increase of the fruit fly, Anastrepha zenildae Zucchi (Diptera: Tephritidae), probably a result of the introduction of irrigated guava orchards that make fruit available all year. Knowledge of the sexual behavior of Tephritidae has great importance to pest control programs, particularly those that employ the Sterile Insect Technique. In order to characterize the reproductive behavior of A. zenildae, 32 individuals (16 males; 16 females) in each of six generations were submitted to an artificial 12:12 L:D cycle (750: < 1 lux, lights on 07:00–19:00) and observed over their lifetimes. The courtship and copulation occurred in leks and the episodes varied with the time of day, courtship being most frequent between Zeitgeber time (ZT) 3 and ZT 7, peaking at ZT 5–6. Copulations occurred between ZT 2 and ZT 8, with a higher frequency between ZT 5–7 and a peak at ZT 6. Mean duration was 0.28 ± 0.03 min/male (range: 5–163 min). Males in the leks attempted to copulate mainly between ZT 3 and ZT 7 with a peak at ZT 6, and males outside leks peaked at ZT 7. The different timing of sexual behaviors among related sympatric species, including A. zenildae, may contribute to species isolation

The southern photometric local universe survey (S-PLUS): Improved SEDs, morphologies, and redshifts with 12 optical filters

The Southern Photometric Local Universe Survey (S-PLUS) is imaging ~9300 deg2 of the celestial sphere in 12 optical bands using a dedicated 0.8mrobotic telescope, the T80-South, at the Cerro Tololo Inter-american Observatory, Chile. The telescope is equipped with a 9.2k × 9.2k e2v detector with 10 μm pixels, resulting in a field of view of 2 deg2 with a plate scale of 0.55 arcsec pixel-1. The survey consists of four main subfields, which include two non-contiguous fields at high Galactic latitudes (|b| > 30° , 8000 deg2) and two areas of the Galactic Disc and Bulge (for an additional 1300 deg2). S-PLUS uses the Javalambre 12-band magnitude system, which includes the 5 ugriz broad-band filters and 7 narrow-band filters centred on prominent stellar spectral features: the Balmer jump/[OII], Ca H + K, Hd, G band, Mg b triplet, Hα, and the Ca triplet. S-PLUS delivers accurate photometric redshifts (δz/(1 + z) = 0.02 or better) for galaxies with r < 19.7 AB mag and z < 0.4, thus producing a 3D map of the local Universe over a volume of more than 1 (Gpc/h)3. The final S-PLUS catalogue will also enable the study of star formation and stellar populations in and around the Milky Way and nearby galaxies, as well as searches for quasars, variable sources, and low-metallicity stars. In this paper we introduce the main characteristics of the survey, illustrated with science verification data highlighting the unique capabilities of S-PLUS. We also present the first public data release of ~336 deg2 of the Stripe 82 area, in 12 bands, to a limiting magnitude of r = 21, available at datalab.noao.edu/splus.Fil: De Oliveira, C. Mendes. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Ribeiro, T.. Universidade Federal de Sergipe; Brasil. National Optical Astronomy Observatory; Estados UnidosFil: Schoenell, W.. Universidade Federal do Rio Grande do Sul; BrasilFil: Kanaan, A.. Universidade Federal de Santa Catarina; BrasilFil: Overzier, R.A.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil. Ministério da Ciência, Tecnologia, Inovação e Comunicações. Observatório Nacional; BrasilFil: Molino, A.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Sampedro, L.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Coelho, P.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Barbosa, C.E.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Cortesi, A.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Costa Duarte, M.V.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Herpich, F.R.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil. Universidade Federal de Santa Catarina; BrasilFil: Hernandez Jimenez, J.A.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Placco, V.M.. University of Notre Dame; Estados Unidos. JINA Center for the Evolution of the Elements ; Estados UnidosFil: Xavier, H.S.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Abramo, L.R.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Saito, R.K.. Universidade Federal de Santa Catarina; BrasilFil: Chies Santos, A.L.. Universidade Federal do Rio Grande do Sul; BrasilFil: Ederoclite, A.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil. Centro de Estudios de Física del Cosmo de Aragon; EspañaFil: De Oliveira, R. Lopes. Universidade Federal de Sergipe; Brasil. Ministério da Ciência, Tecnologia, Inovação e Comunicações. Observatório Nacional; Brasil. University of Maryland; Estados UnidosFil: Goncalves, D.R.. Universidade Federal do Rio de Janeiro; BrasilFil: Akras, S.. Ministério da Ciência, Tecnologia, Inovação e Comunicações. Observatório Nacional; Brasil. Universidade Federal do Rio de Janeiro; BrasilFil: Almeida, L.A.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil. Universidade Federal do Rio Grande do Norte; BrasilFil: Almeida Fernandes, F.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; Brasil. Universidade Federal do Rio de Janeiro; BrasilFil: Beers, T.C.. University of Notre Dame; Estados Unidos. JINA Center for the Evolution of the Elements ; Estados UnidosFil: Bonatto, C.. Universidade Federal do Rio Grande do Sul; BrasilFil: Bonoli, S.. Centro de Estudios de Física del Cosmo de Aragon; EspañaFil: Cypriano, E.S.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Vinicius Lima, E.. Universidade do Sao Paulo. Instituto de Astronomia, Geofísica e Ciências Atmosféricas; BrasilFil: Smith Castelli, Analia Viviana. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Astrofísica La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Astronómicas y Geofísicas. Instituto de Astrofísica La Plata; Argentin