Georgia College & State University

About: Georgia College & State University is a education organization based out in Milledgeville, Georgia, United States. It is known for research contribution in the topics: Population & Context (language use). The organization has 950 authors who have published 1591 publications receiving 37027 citations.

Refusing to Tolerate Intolerance: An Experiment Testing the Link Between Exposure to Gay-Related Content and Resulting Attitudes and Behaviors

Abstract: This article describes a 2 × 2 factorial design experiment with 334 undergraduates testing the influence of exposure to gay-related photographs on endorsement of tolerant gay attitudes and likelihood to interact with the photograph within a social media context. Individuals were more likely to interact with and be attitudinally influenced by pro-gay rather than anti-gay content. Prior media exposure to gay-related content was positively associated with likelihood to interact with the photographs. The experimental condition moderated this association. Our results provide support and extension for social cognitive theory, cultivation, and the heuristic processing model, as well as offer new information related to the study of social media, particularly those current conversational trends related to gay men and lesbians.

Newly Recognized Diversity in Trochodendraceae from the Eocene of Western North America

Abstract: The Eocene flora of the Okanogan Highlands in the Pacific Northwest of North America has been recognized previously to include extinct species of both extant genera of the Trochodendraceae Here, u

Near-infrared spectroscopy of 20 new Chandra sources in the Norma arm

Abstract: We report on CTIO/NEWFIRM and CTIO/OSIRIS photometric and spectroscopic observations of 20 new X-ray (0.5–10 keV) emitters discovered in the Norma arm Region Chandra Survey (NARCS). NEWFIRM photometry was obtained to pinpoint the nearinfrared counterparts of NARCS sources, while OSIRIS spectroscopy was used to help identify 20 sources with possible high mass X-ray binary properties. We find that (1) two sources are WN8 Wolf-Rayet stars, maybe in colliding wind binaries, part of the massive star cluster Mercer 81; (2) two are emission-line stars, possibly in X-ray binaries, that exhibit near- and mid-infrared excesses either due to free-free emission from the decretion discs of Be stars or warm dust in the stellar winds of peculiar massive stars such as B[e] supergiants or luminous blue variables; (3) one is a B8-A3 IV-V star that could be in a quiescent high mass X-ray binary system; (4) two are cataclysmic variables including one intermediate polar; (5) three may be neutron star symbiotic binaries; (6) five are most likely white dwarf symbiotic binaries; and (7) five exhibit properties more consistent with isolated giant/dwarf stars. The possible detection of one to three high mass X-ray binaries is in good agreement with our predictions. However, our study illustrates the difficulty of clearly differentiating quiescent or intermediate X-ray luminosity systems from isolated massive stars, which may lead to an underestimation of the number of known high mass X-ray binaries.