839 resultados para political candidates
Resumo:
Understanding the impact of political violence on child maladjustment is a matter of international concern. Recent research has advanced a social ecological explanation for relations between political violence and child adjustment. However, conclusions are qualified by the lack of longitudinal tests. Toward examining pathways longitudinally, mothers and their adolescents (M = 12.33, SD = 1.78, at Time 1) from 2-parent families in Catholic and Protestant working class neighborhoods in Belfast, Northern Ireland, completed measures assessing multiple levels of a social ecological model. Utilizing autoregressive controls, a 3-wave longitudinal model test (T1, n = 299; T2, n = 248; T3, n = 197) supported a specific pathway linking sectarian community violence, family conflict, childrens insecurity about family relationships, and adjustment problems.
Resumo:
The present research addresses how voters’ perceptions of Hillary Clinton’s warmth and competence influenced decisions to vote for her in the 2008 Democratic primary. We apply research on gender stereotypes and perceptions of women leaders to demonstrate that voters perceived Clinton as highly competent but relatively less warm. Further, this research examines how perceptions of Clinton’s warmth and competence contributed to decisions to vote for her. Results suggest that perceptions of Clinton’s warmth and competence differentially predicted voting behavior for voters strongly and less strongly identified with their political party. This research provides a descriptive analysis of how voters’ beliefs about leaders can be colored by gender, and how such beliefs contribute to electing women candidates.
Resumo:
We have carried out a survey of the Andromeda galaxy for unresolved microlensing (pixel lensing). We present a subset of four short timescale, high signal-to-noise microlensing candidates found by imposing severe selection criteria: the source flux variation exceeds the flux of an R = 21 magnitude star and the full width at half maximum timescale is less than 25 days. Remarkably, in three out of four cases, we have been able to measure or strongly constrain the Einstein crossing time of the event. One event, which lies projected on the M 31 bulge, is almost certainly due to a stellar lens in the bulge of M 31. The other three candidates can be explained either by stars in M 31 and M 32 or by MACHOs.