A History of Financial Aid to Students

The history of financial aid in higher education covers a board range of philanthropic-, scholarship-, and loan-based approaches. This article comprehensively covers the history of American financial aid to students from influences of European medieval institutions to contemporary aid systems. A broad history of financial aid is covered, revealing an evolution from a system primarily based upon local philanthropic efforts, to a more formal system of scholarships and grants, to, finally, a complex federal system of loans. As the history of financial aid is chronologically covered, attention is paid to describing how financial aid policies and practices were a response to societal and political contexts of their times and how need- and merit-based philosophies have given way to political agenda-based philosophies of aid

Does the House Always Win? An Analysis of Barriers to Wealth Building and College Borrowing

The racial differences in student loan debt must be interpreted through a lens of wealth building inequality. Black individuals in particular are negatively affected by official and unofficial policies that create barriers to building wealth. Financial aid policies then exacerbate this inequality with an Expected Family Contribution (EFC) formula that protects the majority of family assets from being used as required educational contributions. Using the 2011-12 National Postsecondary Student Aid Survey (NPSAS:12) , we examined differences in student loan debt based on wealth building barriers (students’ access to banks, father’s education, and mother’s education). Our ANOVA models show cumulative loan debt is highest amongst students who experience barriers to wealth building (students who do not have bank accounts, students whose fathers have less than a Bachelor’s degree, and students whose mothers have less than a Bachelor’s degree) (p \u3c .05). In addition, a greater percentage of black students than white experience these wealth building barriers

Difference in Preparedness: Do School Staff Feel Prepared for an Active Shooter or Attack?

The 2020 Texas Educators’ Needs Assessment Regarding School Safety and Victims Services included responses from educators across the state of Texas regarding school safety. This needs assessment generated data that provided researchers with the unique opportunity to analyze the school safety issues in Texas (Fuller et al, 2020). The purpose of the study was to evaluate Texas K-12 educators responses to their school’s preparedness for an active attack or shooter using data from that needs assessment. To build a strong analysis, the results were separated into three categories: educator role; Texas school regions; and urbanicity. Pearson chi square statistical analysis was used to create an understanding of the data. The results of this analysis revealed a trend that a majority of K-12 educators felt prepared for an active attack or shooter

The former companion of the hyper-velocity star S5-HVS1

The hyper-velocity star S5-HVS1, ejected 5 Myr ago from the Galactic Center at 1800 km/s, was most likely produced by tidal break-up of a tight binary by the supermassive black hole SgrA*. Taking a Monte Carlo approach, we show that the former companion of S5-HVS1 was likely a main-sequence star between 1.5 and 6M⊙ and was captured into a highly eccentric orbit with pericenter distance in the range 1-10 AU and semimajor axis about 10³ AU. We then explore the fate of the captured star. We find that the heat deposited by tidally excited stellar oscillation modes leads to runaway disruption if the pericenter distance is smaller than about 3 AU. Over the past 5 Myr, its angular momentum has been significantly modified by orbital relaxation, which may stochastically drive the pericenter inwards below 3 AU and cause tidal disruption. We find an overall survival probability in the range 5% to 50%, depending on the local relaxation time in the close environment of the captured star, and the initial pericenter at capture. The pericenter distance of the surviving star has migrated to 10-100 AU, making it potentially the most extreme member of the S-star cluster. From the ejection rate of S5-HVS1-like stars, we estimate that there may currently be a few stars in such highly eccentric orbits. They should be detectable (typically K_s ≾18.5 mag) by the GRAVITY instrument and by future Extremely Large Telescopes and hence provide an extraordinary probe of the spin of SgrA*

A new class of large-amplitude radial-mode hot subdwarf pulsators

Using high-cadence observations from the Zwicky Transient Facility at low Galactic latitudes, we have discovered a new class of pulsating, hot compact stars. We have found four candidates, exhibiting blue colors (g − r ≤ −0.1 mag), pulsation amplitudes of >5%, and pulsation periods of 200–475 s. Fourier transforms of the light curves show only one dominant frequency. Phase-resolved spectroscopy for three objects reveals significant radial velocity, T eff, and log(g) variations over the pulsation cycle, which are consistent with large-amplitude radial oscillations. The mean T eff and log(g) for these stars are consistent with hot subdwarf B (sdB) effective temperatures and surface gravities. We calculate evolutionary tracks using MESA and adiabatic pulsations using GYRE for low-mass, helium-core pre-white dwarfs (pre-WDs) and low-mass helium-burning stars. Comparison of low-order radial oscillation mode periods with the observed pulsation periods show better agreement with the pre-WD models. Therefore, we suggest that these new pulsators and blue large-amplitude pulsators (BLAPs) could be members of the same class of pulsators, composed of young ≈0.25–0.35 M ⊙ helium-core pre-WDs.Published versio