Warm HCN, C2H2, and CO in the disk of GV Tau

We present the first high-resolution, ground-based observations of HCN and C2H2 toward the T Tauri binary star system GV Tau. We detected strong absorption due to HCN nu_3 and weak C2H2 (nu_3 and nu_2 + (nu_4 + nu_5)^0_+) absorption toward the primary (GV Tau S) but not the infrared companion. We also report CO column densities and rotational temperatures, and present abundances relative to CO of HCN/CO ~0.6% and C2H2/CO ~1.2% and an upper limit for CH4/CO < 0.37% toward GV Tau S. Neither HCN nor C2H2 were detected toward the infrared companion and results suggest that abundances may differ between the two sources.Comment: 23 pages, 6 figures, accepted by Ap

The Eternal Crossroads: The Art of Flannery O\u27Connor

Flannery O’Connor was a writer of extraordinary power and virtuosity. Her strong supple prose blends humor, pathos, satire, and grotesquerie which leads the reader to the evil at the center of the self’s labyrinth. There, she confronts that evil with originality and power, pulling the reader into consideration of the terrifying dependencies of love in the recesses of the heart. This study focuses on Flannery O’Connor’s sense of the coincidence of the eternal and cosmic with worldly time and place—“the eternal crossroads”— and how that sense controls and infuses her fiction. From an examination of various influences upon Miss O’Connor’s work—Pierre Teilhard de Chardin, Mauriac, Nathaniel West, and Hawthorne—the authors consider her novels and stories, as well as several stories never collected. Their textual analysis shows that her structures, images, motifs, and symbols became vehicles for anagogical meaning as she progressed from early promise to artistic fulfillment. Considering O’Connor’s own comments on her writing, the authors illuminate some frequently misunderstood features of her work, such as her “grotesques” and her stress on death and violence. In so doing they make an important contribution to our understanding of how Flannery O’Connor arrived at “the eternal crossroads.” Leon V. Driskell teaches English at the University of Louisville, and Joan T. Brittain teaches English at Bellarmine- Ursuline College.https://uknowledge.uky.edu/upk_english_language_and_literature_north_america/1023/thumbnail.jp

Responses of Vascular Endothelial Cells to Photoembossed Topographies on Poly(Methyl Methacrylate) Films.

Failures of vascular grafts are normally caused by the lack of a durable and adherent endothelium covering the graft which leads to thrombus and neointima formation. A promising approach to overcome these issues is to create a functional, quiescent monolayer of endothelial cells on the surface of implants. The present study reports for the first time on the use of photoembossing as a technique to create polymer films with different topographical features for improved cell interaction in biomedical applications. For this, a photopolymer is created by mixing poly(methyl methacrylate) (PMMA) and trimethylolpropane ethoxylate triacrylate (TPETA) at a 1:1 ratio. This photopolymer demonstrated an improvement in biocompatibility over PMMA which is already known to be biocompatible and has been extensively used in the biomedical field. Additionally, photoembossed films showed significantly improved cell attachment and proliferation compared to their non-embossed counterparts. Surface texturing consisted of grooves of different pitches (6, 10, and 20 µm) and heights (1 µm and 2.5 µm). The 20 µm pitch photoembossed films significantly accelerated cell migration in a wound-healing assay, while films with a 6 µm pitch inhibited cells from detaching. Additionally, the relief structure obtained by photoembossing also changed the surface wettability of the substrates. Photoembossed PMMA-TPETA systems benefited from this change as it improved their water contact angle to around 70°, making it well suited for cell adhesion.This project was supported in part by MRC/EPSRC grant G0502256-77947. Lin Qiu was supported by a joint PhD studentship from Queen Mary University of London and the China Scholarship Council (CSC) between 2010 and 2014

Erratum: Warm HCN, C2H2, and CO in the Disk of GV Tau\u27\u27

This is an Erratum for the article 2007 ApJ 660 157

Near-Infrared Spectroscopic Study of V1647 Ori

We present new high-resolution infrared echelle spectra of V1647 Ori, the young star that illuminates McNeil\u27s nebula. From the start, V1647 Ori has been an enigmatic source that has defied classification, in some ways resembling eruptive stars of the FUor class and in other respects the EXor variables. V1647 Ori underwent an outburst in 2003 before fading back to its pre-outburst brightness in 2006. In 2008, it underwent a new outburst. In this paper we present high-resolution K-band and M-band spectra from the W. M. Keck Observatory that were acquired during the 2008 outburst. We compare the spectra to spectra acquired during the previous outburst and quiescent phases. We find that the luminosity and full width at half maximum power of Br-gamma increased as the star has brightened and decreased when the star faded indicating that these phases are driven by variations in the accretion rate. We also show that the temperature of the CO emission has varied with the stellar accretion rate confirming suggestions from modeling of the heating mechanisms of the inner disk (e.g. Glassgold et al. 2004). Finally we find that the lowest energy blue-shifted CO absorption lines originally reported in 2007 are no longer detected. The absence of these lines confirms the short-lived nature of the outflow launched at the start of the quiescent phase in 2006