From stopout to scholar : pathways to graduation through adult degree completion programs.

Although colleges and universities are facing increased scrutiny to demonstrate a return on investment for their students, the demand for college-educated workers continues to grow. As of 2010, the U.S. Census Bureau estimated that more than one-fifth of Americans age 25 and older—around 43.5 million people—have some postsecondary education but no degree (Lumina, 2012). This article presents an integrative review of relevant, rigorous, and research based programs that create a fast path to degree completion for working adults. While national data still shows that postsecondary credentials remain a good investment for individuals and the overall economy (Carnavale & Rose, 2015), the public is asserting a greater demand for accountability as tuition continues to escalate well beyond the rate of inflation. This article provides a review and conceptual links to educational pathways for the large group of adult learners with some college and no degree

Unpacking organizational alignment : the view from theory and practice.

The importance of alignment is widely acknowledged in organizations. Yet, we know little about how alignment is created or measured over time at multiple levels in the organization. This paper attempts to expand and enrich different perspectives and types of alignment that exist and occur in organizations. Throughout, we elaborate on how organizational alignment is understood and defined in the extant literature. Next, we propose a framework for examining different perspectives of organizational alignment emphasizing conceptual similarities as well as distinctiveness. Our core contribution is an emergent theoretical framework that expands on the concept of organizational alignment. We find that while conceptual overlap is problematic from a theory building perspective, the organizational context of alignment necessitates unique and varying ways in which this construct is practiced. We apply the theoretical framework to develop recommendations for senior leaders, human resource and operations managers. Finally, we present implications for both theory and practice

A Deficiency of Donors or an Abundance of Barriers? Title IX Fundraising Challenges from the Perspective of Athletic Department Fundraisers

This paper explores how Title IX effects college athletic fundraising, particularly how athletic fundraisers creates an unfair environment for non-football and basketball programs. Using distributive justice as a theoretical lens, we examine the perspective of athletic department fundraisers working at NCAA, Power Five athletic departments. Interviews from participants gleaned insights into only meeting the minimum legal requirements of Title IX, fighting between non-revenue programs for remaining resources, elevated requirements for program success for non-football and basketball programs, and more. This paper aims at providing insight into a distinct context of fundraising, which often avoids Title IX scrutiny, but is the primary outlet for athletic departments to raise additional funds for their sport programs

Analysis of Base Heating Environment During Ground Testing of a Lunar Lander Demonstrator

Introduction: This lunar lander demonstrator, known as XL-1T (terrestrial), is a collaborative effort between Masten Space Systems and NASA, under NASAs Lunar CATALYST (also known as Lunar Cargo Transportation and Landing by Soft Touchdown) initiative; The lunar lander is a reusable terrestrial test bed for Mastens powered decent landing system, and will be controlled by four throttleable main engines utilizing green hypergolic propellants; One of the concerns for a four-engine vehicle like this demonstrator, is the potential for a severe base-heating environment, caused by the formation of a fountain jet during testing. Fountain jet is an unique base flow physics which was discovered during the development of the DC-X vehicle

N-band Imaging of Seyfert Nuclei and the MIR-X-ray correlation

We present new mid-infrared (N-band) images of a sample of eight nearby Seyfert galaxies. In all of our targets, we detect a central unresolved source, which in some cases has been identified for the first time. In particular, we have detected the mid-infrared emission from the active nucleus of NGC 4945, which previously remained undetected at any wavelength but hard X-rays. We also detect circumnuclear extended emission in the Circinus galaxy along its major axis, and find marginal evidence for extended circumnuclear emission in NGC 3281. The high spatial resolution (1.7") of our data allows us to separate the flux of the nuclear point sources from the extended circumnuclear starburst (if present). We complement our sample with literature data for a number of non-active starburst galaxies, and relate the nuclear N-band flux to published hard (2-10 kev) X-ray fluxes. We find tight and well-separated correlations between nuclear N-band flux and X-ray flux for both Seyfert and starburst nuclei which span over 3 orders of magnitude in luminosity. We demonstrate that these correlations can be used as a powerful classification tool for galactic nuclei. For example, we find strong evidence against NGC 1808 currently harbouring an active Seyfert nucleus based on its position in the mid-infrared-X-ray diagram. On the other hand, we confirm that NGC 4945 is in fact a Seyfert 2 galaxy.Comment: 31 pages, incl. 4 figures, uses AASTex. Replaced with accepted version after minor modifications. To appear in Ap

X Her and TX Psc: Two cases of ISM interaction with stellar winds observed by Herschel

The asymptotic giant branch (AGB) stars X Her and TX Psc have been imaged at 70 and 160 microns with the PACS instrument onboard the Herschel satellite, as part of the large MESS (Mass loss of Evolved StarS) Guaranteed Time Key Program. The images reveal an axisymmetric extended structure with its axis oriented along the space motion of the stars. This extended structure is very likely to be shaped by the interaction of the wind ejected by the AGB star with the surrounding interstellar medium (ISM). As predicted by numerical simulations, the detailed structure of the wind-ISM interface depends upon the relative velocity between star+wind and the ISM, which is large for these two stars (108 and 55 km/s for X Her and TX Psc, respectively). In both cases, there is a compact blob upstream whose origin is not fully elucidated, but that could be the signature of some instability in the wind-ISM shock. Deconvolved images of X Her and TX Psc reveal several discrete structures along the outermost filaments, which could be Kelvin-Helmholtz vortices. Finally, TX Psc is surrounded by an almost circular ring (the signature of the termination shock?) that contrasts with the outer, more structured filaments. A similar inner circular structure seems to be present in X Her as well, albeit less clearly.Comment: 11 pages, Astronomy & Astrophysics, in pres

Brass Happenings

Presenting a student recital for brass students in USU\u27s Music Department.https://digitalcommons.usu.edu/music_programs/1107/thumbnail.jp