Girl Connection, November 2008

A monthly newsletter for Iowa Commission on the Status of Women

Girl Connection, February 2009

A monthly newsletter for Iowa Commission on the Status of Women

Girl Connection, June 2009

A monthly newsletter for Iowa Commission on the Status of Women. Teens, Sex and Technology

Is the capture success of orchid bees (Hymenoptera, Apoidea) influenced by different baited trap designs? A case study from southern Brazil

Orchid bees are increasingly applied on Neotropical biomonitoring and bioindication studies due to the relative easiness of sampling and identification when compared to other bee groups. A considerable number of orchid bee community studies have been adopting baited traps as a sampling method, especially for replication purposes. However, the trap attributes are variable, and hitherto no evaluation of different designs was carried out. Here, five attributes of baited traps were tested: trap volume, number of entrance holes, presence of landing platform, kind of landing platform, and fixation content. We use Mann-Whitney tests to access differences in richness and abundance capture rates for each trap design. We found that volume, number of entrance holes, and fixation content do not influence orchid bees capture. However, the design without landing platforms had a significantly higher capture rate for richness when compared with sanded landing platforms. On the other hand, analyzing the kind of landing platform, we detected a significantly higher richness and abundance for the trap with landing platforms glued with sand. Despite the fact that the effects of different designs tested here were very punctual, we consider that results from samples taken with different baited trap designs are comparable. Some adjustments on trap design can be done according to the particularities of future studies.

Girl Connection, August 2009

A monthly newsletter for Iowa Commission on the Status of Women. Relationship Bridge

Girl Connection, October 2009

A monthly newsletter for Iowa Commission on the Status of Women. 11 Components of Female Responsive Practice

Girl Connection, December 2009

A monthly newsletter for Iowa Commission on the Status of Women. 11 Components of Female Responsive Practice

Girl Connection, February 2010

A monthly newsletter for Iowa Commission on the Status of Women; Anxiety and Economic Uncertainty

Exploring the connection between the stellar wind and the non-thermal emission in LS 5039

Context.LS 5039 has been observed with several X-ray instruments so far showing quite steady emission in the long term and no signatures of accretion disk. The source also presents X-ray variability at orbital timescales in flux and photon index. The system harbors an O-type main sequence star with moderate mass-loss. At present, the link between the X-rays and the stellar wind is unclear. Aims.We study the X-ray fluxes, spectra, and absorption properties of LS 5039 at apastron and periastron passages during an epoch of enhanced stellar mass-loss, and the long term evolution of the latter in connection with the X-ray fluxes. Methods.New XMM-Newton observations were performed around periastron and apastron passages in September 2005, when the stellar wind activity was apparently higher. April 2005 Chandra observations on LS 5039 were revisited. Moreover, a compilation of H EW data obtained since 1992, from which the stellar mass-loss evolution can be approximately inferred, was carried out. Results.XMM-Newton observations show higher and harder emission around apastron than around periastron. No signatures of thermal emission or a reflection iron line indicating the presence of an accretion disk are found in the spectrum, and the hydrogen column density () is compatible with being the same in both observations and consistent with the interstellar value. 2005 Chandra observations show a hard X-ray spectrum, and possibly high fluxes, although pileup effects preclude conclusive results from being obtained. The H EW shows yearly variations of 10%, and does not seem to be correlated with X-ray fluxes obtained at similar phases, unlike what is expected in the wind accretion scenario. Conclusions.2005 XMM-Newton and Chandra observations are consistent with 2003 RXTE/PCA results, namely moderate flux and spectral variability at different orbital phases. The constancy of the seems to imply that either the X-ray emitter is located at 1012 cm from the compact object, or the density in the system is 3 to 27 times smaller than that predicted by a spherical symmetric wind model. We suggest that the multiwavelength non-thermal emission of LS 5039 is related to the observed extended radio jets and is unlikely to be produced inside the binary system.

Girl Connection, April 2010

A monthly newsletter for Iowa Commission on the Status of Women; Anxiety and Economic Uncertainty

Girl Connection, June 2010

A monthly newsletter for Iowa Commission on the Status of Women; Anxiety and Economic Uncertainty

Girl Connection, August 2010

A monthly newsletter for Iowa Commission on the Status of Women; Anxiety and Economic Uncertainty

Girl Connection, October 2010

A monthly newsletter for Iowa Commission on the Status of Women; Anxiety and Economic Uncertainty