9,299 research outputs found
Making Family Under A Shiftwork Schedule: Air Force Security Guards And Their Wives
Through 90 in-depth interviews with 44 rotating shiftworkers and their spouses, this study examines how couples adjust their routines in order to interact as a family unit. We suggest that their views of marital roles are a critical force shaping their practices of daily family life. Wives, even when employed, are responsible for coordinating the individual schedules of family members to match that of the shift-working husband. Wives pay a price for this adjustment work in the form of biological, and emotional symptoms similar to those previously reported only for shiftworkers. Despite their efforts to be providers, husbands pay a price in terms of guilt and anger when work demands limit their ability to fully participate in family life. Further, dual-earner couples rely on husbands ( father care ) and informal arrangements to cover child care for economical and social reasons, not simply to provide husbands with an opportunity to interact with children. Yet, despite higher levels of father care, traditional gender roles have not been altered in that working wives still retain primary responsibility for children
An electrothermally actuated micro valve
Microminiature slide action valve requires power only during actuation and can be used as an on-off or single inlet to alternately selected outlets
The Milky Way halo as a QSO absorption-line system. New results from an HST/STIS absorption-line catalogue of Galactic high-velocity clouds
We use archival UV absorption-line data from HST/STIS to statistically
analyse the absorption characteristics of the high-velocity clouds (HVCs) in
the Galactic halo towards more than 40 extragalactic background sources. We
determine absorption covering fractions of low- and intermediate ions (OI, CII,
SiIII, MgII, FeII, SiIII, CIV, and SiIV) in the range fc = 0.20 - 0.70. For
detailed analysis we concentrate on SiII absorption components in HVCs, for
which we investigate the distribution of column densities, b-values, and radial
velocities. Combining information for SiII and MgII, and using a geometrical
HVC model we investigate the contribution of HVCs to the absorption cross
section of strong MgII absorbers in the local Universe. We estimate that the
Galactic HVCs would contribute on average ~52 % to the total strong MgII cross
section of the Milky Way, if our Galaxy were to be observed from an exterior
vantage point. We further estimate that the mean projected covering fraction of
strong MgII absorption in the Milky Way halo and disc from an exterior vantage
point is fc(sMgII) = 0.31 for a halo radius of R = 61 kpc. These numbers,
together with the observed number density of strong MgII absorbers at low
redshift, indicate that the contribution of infalling gas clouds (i.e., HVC
analogues) in the halos of Milky Way-type galaxies to the cross section of
strong MgII absorbers is <34 %. These findings are in line with the idea that
outflowing gas (e.g., produced by galactic winds) in the halos of more actively
star-forming galaxies dominate the absorption-cross section of strong MgII
absorbers in the local Universe
A Survey of Analogs to Weak MgII Absorbers in the Present
We present the results of a survey of the analogs of weak MgII absorbers
(rest frame equivalent width W(2796) < 0.3 A) at 0 < z < 0.3. Our sample
consisted of 25 HST/STIS echelle quasar spectra (R = 45,000) which covered SiII
1260 and CII 1335 over this redshift range. Using those similar transitions as
tracers of MgII facilitates a much larger survey, covering a redshift
pathlength of g(z) = 5.3 for an equivalent width limit of MgII corresponding to
W(2796) > 0.02 A, with 30% completeness for the weakest lines. We find the
number of weak MgII absorber analogs with 0.02 < W(2796) < 0.3 to be dN/dz =
1.00 +/- 0.20 for 0 < z < 0.3. This value is consistent with cosmological
evolution of the population. We consider the expected effect on observability
of weak MgII absorbers of the decreasing intensity of the extragalactic
background radiation eld from z~1 to z~0. Assuming that all the objects that
produce absorption at z~1 are stable on a cosmological timescale, and that no
new objects are created, we would expect dN/dz of 2-3 at z~0. About 30-50% of
this z~0 population would be decendants of the parsec-scale structures that
produce single-cloud, weak MgII absorbers at z~1. The other 50-70% would be
lower density, kiloparsec-scale structures that produce CIV absorption, but not
detectable low ionization absorption, at z~1. We conclude that at least one,
and perhaps some fraction of both, of these populations has evolved away since
z~1, in order to match the z~0 dN/dz measured in our survey. This would follow
naturally for a population of transient structures whose generation is related
to star-forming processes, whose rate has decreased since z~1.Comment: 45 pages, 12 figures, 7 tables ApJ accepte
Primaquine sensitivity: Some epidemiological and biochemical aspects
.A Thesis presented for the degree of Doctor of Medicine at the University of the Witwatersrand
SEPTEMBER 1962.Plasmoquine (piasmochin, paiuaquin) was the first synthetic antimalarial drug, and it aroused a great deal of interest when it became available in 1926. Dixon (1933) estimated that at least 415 papers relating to plasmoquine hid appeared in the first 4 years following iti introduction, thereafter the volume of communications decreased somewhat,until fresh interest was stimulated by the Second world <.ar and the horean »,ar with fighting in maiariou. areasIT201
Integrated waveguide and nanostructured sensor platform for surface-enhanced Raman spectroscopy
Limitations of current sensors include large dimensions, sometimes limited sensitivity and inherent single-parameter measurement capability. Surface-enhanced Raman spectroscopy can be utilized for environment and pharmaceutical applications with the intensity of the Raman scattering enhanced by a factor of 106. By fabricating and characterizing an integrated optical waveguide beneath a nanostructured precious metal coated surface a new surface-enhanced Raman spectroscopy sensing arrangement can be achieved. Nanostructured sensors can provide both multiparameter and high-resolution sensing. Using the slab waveguide core to interrogate the nanostructures at the base allows for the emission to reach discrete sensing areas effectively and should provide ideal parameters for maximum Raman interactions. Thin slab waveguide films of silicon oxynitride were etched and gold coated to create localized nanostructured sensing areas of various pitch, diameter, and shape. These were interrogated using a Ti:Sapphire laser tuned to 785-nm end coupled into the slab waveguide. The nanostructured sensors vertically projected a Raman signal, which was used to actively detect a thin layer of benzyl mercaptan attached to the sensors
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