Lay Shepherding: Developing a Pastoral Care Ministry for the Small to Mid-Sized Church

A survey of Wesleyan churches and a review of current literature reveals that most pastors are bearing the burden of pastoral care alone. Only a few churches are effectively equipping and empowering lay persons to help provide this needed and meaningful ministry within the body of Christ. The purpose of this project is to demonstrate biblically and historically that the laity are gifted for ministry and that they are called to the task of shepherding God\u27s flock. Further, this project seeks to present a model for implementing a lay shepherding ministry in the small to mid-sized church

Energy Cultures policy briefs

Launched in 2012, the Energy Cultures Project is led by the Centre for Sustainability at the University of Otago and aims to develop knowledge and tools to achieve a sustainable energy transition across New Zealand. The Energy Cultures 2 Project focuses on efficiency transitions in three domains: households, businesses and transport systems.These policy briefs are an output of the Energy Cultures 2 research programme, funded 2012-2016 by the Ministry of Business, Innovation and Employment. The purpose of these briefs is to assist with the design of improved policies and practices to promote more efficient energy use in households, businesses and transport in New Zealand

Spectro-interferometric observations of classical nova V458 Vul 2007

We used the Palomar Testbed Interferometer (PTI) to resolve 2.2 $\mu$m emission from the classical nova V458 Vul 2007 over the course of several days following its discovery on 2007 August 8.54 UT. We also obtained K-band photometric data and spectra of the nova during the early days of the outburst. We also used photometric measurements from the AAVSO database. This is a unique data set offering a 3-technique approach: high-resolution imaging, spectroscopy and photometry. Our analysis shows that the nova ejecta can be modeled as an inclined disk at low inclination i.e. low ellipticity which is consistent with the nova being in the fireball phase at which the outflowing gas is optically thick, confirmed by the presence of strong P-Cygni Balmer lines in the spectra. The expansion velocity is $\approx$1700 $\rm km\ s^{-1}$, derived from the H$\alpha$ line. By combining the nova's angular expansion rate measured by PTI with the expansion rate measured from spectroscopy, the inferred distance to the nova is 9.9-11.4 kpc. We also used the K-band fluxes and the derived size of the emission to estimate the total mass ejected from the nova $\approx 4\times 10^{-4} M_{\odot}$. The quick transition of the nova from Fe II to He/N class makes V458 Vul 2007 a hybrid nova.Comment: 31 pages, 7 figures, accepted for publication in Ap