Widowhood and the end of spousal caregiving: Wear and tear or relief?

This paper analyses the impact of spousal care-giving on survivors’ depressive symptoms six months into widowhood, and examines the applicability of a ‘ relief model’ of spousal adjustment during bereavement. We examine several aspects of the care-giving situation, including care-giver stress, care-giving demands, and type and duration of care and how these affect survivors’ depressive symptomatology. The sample is drawn from two waves of the Changing Lives of Older Couples (CLOC) survey, which was conducted in the United States in the Detroit Metropolitan Area, Michigan. The first wave of data was collected from couples and the second from the surviving spouse six months after the death of the partner. We use multiple regression analysis to examine the effects of key variables on depressive symptoms six months into widowhood, controlling for various demographic characteristics and personal circumstances. The results demonstrate that the duration of care-giving is the most influential predictor of survivors’ depressive symptoms six months after the death. Indeed, long-term care-givers experience greater relief than both non-caregivers and short-term care-givers, as the predicted probabilities indicate. The results lead us to emphasise that care-giving and spousal bereavement should be studied as related processes rather than distinct phenomena. Indeed, relief from a chronically stressful care situation may actually ameliorate the negative effect of spousal loss for survivors

Gendered disparities in take-ups of employee health benefits

Using a sample of 2,271 workers from the 2002 National Study of the Changing Workforce whose employers offered personal health insurance, this article investigates the gendered nature of health insurance benefit take-ups. These analyses include family and employment characteristics in addition to employers’ contributions to health insurance premiums, a measure that is unexamined in sociological analyses of health benefits. Progressive logistic regression models predict the effects of gender and family characteristics. Results indicate that women with employed spouses are less likely to take up their own health benefits than are comparable men, net of basic employment characteristics. Gender differences disappear, however, when controlling for the level of employer contributions: women and men are equally likely to draw on their own employer’s health benefits once we account for their out-of-pocket expense. The authors conclude that family contexts and employment structures jointly influence individuals’ choices about their health benefits. The gendered structure of employment and, specifically, gendered patterns in employer contributions to health benefits are a better explanation for women’s lower chances of benefit take-ups than gender relations within families

The development of thirty self-administering and self-scoring elaborative thinking exercises

Thesis (Ed.M.)--Boston Universit

Far infrared maps of the ridge between OMC-1 and OMC-2

Dust continuum emission from a 6 ft x 20 ft region surrounding OMC-1 and OMC-2 were mapped at 55 and 125 microns with 4 ft resolution. The dominant features of the maps are a strong peak at OMC-1 and a ridge of lower surface brightness between OMC-1 and OMC-2. Along the ridge the infrared flux densities and the color temperature decreases smoothly from OMC-1 to OMC-2. OMC-1 is heated primarily by several optical and infrared stars situated within or just at the boundary of the cloud. At the region of minimum column density between OMC-1 and OMC-2 the nearby B0.5 V star NU Ori may contribute significantly to the dust heating. Near OMC-2 dust column densities are large enough so that, in addition to the OMC-2 infrared cluster, the nonlocal infrared sources associated with OMC-1 and NU Ori can contribute to the heating

L1551NE - Discovery of a Binary Companion

L1551NE is a very young (class 0 or I) low-mass protostar located close to the well-studied L1551 IRS5. We present here evidence, from 1.3mm continuum interferometric observations at ~1'' resolution, for a binary companion to L1551NE. The companion, whose 1.3mm flux density is ~1/3 that of the primary component, is located 1.43'' (~230 A.U. at 160pc) to the southeast. The millimeterwave emission from the primary component may have been just barely resolved, with deconvolved size ~0.82"x0.70" (~131x112 A.U.). The companion emission was unresolved (<100 A.U.). The pair is embedded within a flattened circum-binary envelope of size ~5.4'' x 2.3'' (~860 x 370 A.U.). The masses of the three components (i.e. from the cicumstellar material of the primary star and its companion, and the envelope) are approximately 0.044, 0.014 and 0.023 Mo respectively.Comment: 8 pages, 1 figur

Far infrared and submillimeter brightness temperatures of the giant planets

The brightness temperatures of Jupiter, Saturn, Uranus, and Neptune in the range 35 to 1000 micron. The effective temperatures derived from the measurements, supplemented by shorter wavelength Voyager data for Jupiter and Saturn, are 126.8 + or - 4.5 K, 93.4 + or - 3.3 K, 58.3 + or - 2.0 K, and 60.3 + or - 2.0 K, respectively. The implications of the measurements for bolometric output and for atmospheric structure and composition are discussed. The temperature spectrum of Jupiter shows a strong peak at approx. 350 microns followed by a deep valley at approx. 450 to 500 microns. Spectra derived from model atmospheres qualitatively reproduced these features but do not fit the data closely

Engaging Families and the Community in Schools

This module is designed to lead a collaborative group of educators through the process of designing and implementing an event or activity to increase the levels of family and community engagement in schools. The module presents current research supporting family and community involvement in schools. Learners are prepared to recognize potential barriers to increasing family and community involvement and methods to overcome those barriers. Visit professional learning module.https://digitalcommons.gardner-webb.edu/improve/1011/thumbnail.jp

Neutral carbon in the Egg Nebula (AFGL 2688)

A search for sub-mm C I emission from seven stars that are surrounded by dense molecular gas shells led to the detection, in the case of the "Egg Nebula' (AFGL 2688), of an 0.9 K line implying a C I/CO value greater than 5. The material surrounding this star must be extremely carbon-rich, and it is suggested that the apparently greater extent of the C I emission region may be due to the effects of the galactic UV field on the shell's chemistry, as suggested by Huggins and Glassgold (1982)

Focused laser Doppler velocimeter

A system for remotely measuring velocities present in discrete volumes of air is described. A CO2 laser beam is focused by a telescope at such a volume, a focal volume, and within the focusable range, near field, of the telescope. The back scatter, or reflected light, principally from the focal volume, passes back through the telescope and is frequency compared with the original frequency of the laser, and the difference frequency or frequencies represent particle velocities in that focal volume