Psychotherapy and Counseling with Minorities: A Cognitive Approach to Individual and Cultural Differences, by Manuel Ramirez III

La presente investigación tiene el propósito de demostrar cómo a través de una red social conocida como Facebook, mediante su plataforma de fanpage, puede servir como herramienta táctica de convocatoria para que los movimientos sociales generen grandes marchas multitudinarias en la ciudad de Lima durante el año 2017. Siendo un estudio no experimental con diseño transeccional. La población y muestra está formada por los participantes de la red social Facebook dentro de los fanpage. La técnica fue la observación y la entrevista y como instrumentos la ficha de observación y la guía de entrevista. Los resultados indican que Se hallaron 349 funciones del lenguaje en todos los estados de los fanpages. Siendo la función apelativa y referencial las más utilizadas por estos movimientos en un 87,11 %; mientras que la metalingüística y la fática no se emplearon en ningún momento. Asimismo, y en menor cantidad se usaron la función expresiva y la función poética teniendo un 11.17 % y 1.72 % respectivamente. Cabe resaltar, que en reiteradas ocasiones los estados de los fanpages contenían más de una función del lenguaje, llegando a tener hasta las 4 funciones combinadas en un solo estado. Se concluye que las fanpage son utilizadas como herramienta de convocatoria de movimientos sociales mediante mensajes a través de sus estados, imágenes y videos

Radiosensitization of melanoma cells through combined inhibition of protein regulators of cell survival

The incidence of melanoma continues to dramatically increase in most Western countries with predominantly Caucasian populations. However, only limited therapies for the metastatic stage of the disease are currently available. The main purpose of this study is to determine approaches that can substantially increase radiosensitivity of melanoma cells. The PI3K-AKT, NF-κB and COX-2 pathways, which are involved in the radioprotective response, are highly active in melanoma cells. Pharmacological suppression of COX-2 and PI3K-AKT, or RNAi-mediated knockdown of COX-2, substantially increased levels of G2/M arrest of the cell cycle and decreased clonogenic survival of gamma-irradiated melanomas, predominantly via a necrotic mechanism. On the other hand, resveratrol, a polyphenolic phytoalexin, selectively targets numerous cell signaling pathways, decreasing clonogenic survival primarily via an apoptotic mechanism. In melanoma cells, resveratrol inhibits STAT3 and NF-κB-dependent transcription, culminating in suppression of cFLIP and Bcl-xL expression, while activating the MAPK- and the ATM-Chk2-p53 pathways. Resveratrol also upregulates TRAIL promoter activity and induces TRAIL surface expression in some melanoma cell lines, resulting in a rapid development of apoptosis. Sequential treatment of melanoma cells, first with γ-irradiation to upregulate TRAIL-R surface expression, and then with resveratrol to suppress antiapoptotic proteins cFLIP and Bcl-xL and induce TRAIL surface expression, had dramatic effects on upregulation of apoptosis in some melanoma lines, including SW1 and WM35. However, for melanoma lines exhibiting suppressed translocation of TRAIL to the cell surface, a necrotic mechanism of cell death was primarily involved in radiation response. Hence, surface expression of TRAIL induced by resveratrol appears to be a decisive event, one which determines an apoptotic versus a necrotic response of melanoma cells to sequential treatment

KH 15D: A Spectroscopic Binary

We present the results of a high-resolution spectroscopic monitoring program of the eclipsing pre-main-sequence star KH 15D that reveal it to be a single-line spectroscopic binary. We find that the best-fit Keplerian model has a period P = 48.38 days, which is nearly identical to the photometric period. Thus, we find the best explanation for the periodic dimming of KH 15D is that the binary motion carries the currently visible star alternately above and below the edge of an obscuring cloud. The data are consistent with the models involving an inclined circumstellar disk, as recently proposed by Winn et al. (2004) and Chiang & Murray-Clay (2004). We show that the mass ratio expected from models of PMS evolution, together with the mass constraints for the visible star, restrict the orbital eccentricity to 0.68 < e < 0.80 and the mass function to 0.125 < Fm < 0.5 Msun.Comment: 8 pages, 4 figures, 3 tables, accepted for publication in September AJ. Discussion of rotational velocity deferred to Hamilton, et al. (2004, in prep). Previously reported vsini value in error; Replaced Table 3 with new Figure 3; Added new Table 2 showing individual radial velocities w.r.t. each reference star; Fixed typo in Figure

Precise Measures of Orbital Period, Before and After Nova Eruption for QZ Aurigae

For the ordinary classical nova QZ Aurigae (which erupted in 1964), we report 1317 magnitudes from 1912--2016, including four eclipses detected on archival photographic plates from long before the eruption. We have accurate and robust measures of the orbital period both pre-eruption and post-eruption, and we find that the orbital period decreased, with a fractional change of -290.71+-0.28 parts-per-million across the eruption, with the orbit necessarily getting smaller. Further, we find that the light curve outside of eclipses and eruption is flat at near B=17.14 from 1912--1981, whereupon the average light curve starts fading down to B=17.49 with large variability. QZ Aur is a robust counter-example against the Hibernation model for the evolution of cataclysmic variables, where the model requires that all novae have their period increase across eruptions. Large period decreases across eruptions can easily arise from mass imbalances in the ejecta, as are commonly seen in asymmetric nova shells.Comment: MNRAS in press, 24 pages, 5 tables, 6 figure

Chemical Analysis of Five Red Giants in the Globular Cluster M10 (NGC 6254)

We have determined Al, $\alpha$, Fe-peak, and neutron capture elemental abundances for five red giant branch (RGB) stars in the Galactic globular cluster M10. Abundances were determined using equivalent width analyses of moderate resolution (R$\sim$15,000) spectra obtained with the Hydra multifiber positioner and bench spectrograph on the WIYN telescope. The data sample the upper RGB from the luminosity level near the horizontal branch to about 0.5 mag below the RGB tip. We find in agreement with previous studies that M10 is moderately metal-poor with [Fe/H]=-1.45 ($\sigma$=0.04). All stars appear enhanced in Al with =+0.33 ($\sigma$=0.19), but no stars have [Al/Fe]$\ga$+0.55. We find the $\alpha$ elements to be enhanced by +0.20 to +0.40 dex and the Fe--peak elements to have [el/Fe]$\sim$0, which are consistent with predictions from type II SN ejecta. Additionally, the cluster appears to be r-process rich with =+0.41.Comment: 16 Pages; 3 Figures; 3 Tables; Accepted for publication in PAS

A Prograde, Low-Inclination Orbit for the Very Hot Jupiter WASP-3b

We present new spectroscopic and photometric observations of the transiting exoplanetary system WASP-3. Spectra obtained during two separate transits exhibit the Rossiter-McLaughlin (RM) effect and allow us to estimate the sky-projected angle between the planetary orbital axis and the stellar rotation axis, lambda = 3.3^{+2.5}_{-4.4} degrees. This alignment between the axes suggests that WASP-3b has a low orbital inclination relative to the equatorial plane of its parent star. During our first night of spectroscopic measurements, we observed an unexpected redshift briefly exceeding the expected sum of the orbital and RM velocities by 140 m/s. This anomaly could represent the occultation of material erupting from the stellar photosphere, although it is more likely to be an artifact caused by moonlight scattered into the spectrograph.Comment: 23 pages, 4 figures, Accepted for publication in The Astrophysical Journal, Replacement includes revised citation

Enhanced Approaches for Identifying Amadori Products: Application to Peanut Allergens

The dry roasting of peanuts is suggested to influence allergic sensitization as a result of the formation of advanced glycation end products (AGEs) on peanut proteins. Identifying AGEs is technically challenging. The AGEs of a peanut allergen were probed with nano-scale liquid chromatography−electrospray ionization−mass spectrometry (nanoLC−ESI−MS) and tandem mass spectrometry (MS/MS) analyses. Amadori product ions matched to expected peptides and yielded fragments that included a loss of three waters and HCHO. As a result of the paucity of b and y ions in the MS/MS spectrum, standard search algorithms do not perform well. Reactions with isotopically labeled sugars confirmed that the peptides contained Amadori products. An algorithm was developed on the basis of information content (Shannon entropy) and the loss of water and HCHO. Results with test data show that the algorithm finds the correct spectra with high precision, reducing the time needed to manually inspect data. Computational and technical improvements allowed for better identification of the chemical differences between modified and unmodified proteins

Two Jovian-Mass Planets in Earthlike Orbits

We report the discovery of two new planets: a 1.94 M_Jup planet in a 1.8-year orbit of HD 5319, and a 2.51 M_Jup planet in a 1.1-year orbit of HD 75898. The measured eccentricities are 0.12 for HD 5319 b and 0.10 for HD 75898 b, and Markov Chain Monte Carlo simulations based on derived orbital parameters indicate that the radial velocities of both stars are consistent with circular planet orbits. With low eccentricity and 1 < a < 2 AU, our new planets have orbits similar to terrestrial planets in the solar system. The radial velocity residuals of both stars have significant trends, likely arising from substellar or low-mass stellar companions.Comment: 32 pages, including 11 figures and 5 tables. Accepted by Ap