2,112 research outputs found
Alien Registration- Lumsden, Joseph E. (South Portland, Cumberland County)
https://digitalmaine.com/alien_docs/20088/thumbnail.jp
Alien Registration- Lumsden, Annie E. (Bangor, Penobscot County)
https://digitalmaine.com/alien_docs/11793/thumbnail.jp
“They needed the attention more than I did”: how do the birth children of foster carers experience the relationship with their parents?
Research has demonstrated that there is more likely to be a disruption to the placement where foster carers have birth children living at home. Given the limited presence of the birth children of foster carers in research and the importance of the retention of carers, it seems relevant to policy and practice to investigate the parent-child relationship in this context. Therefore, this study aimed to explore how the birth children of foster carers experienced their relationship with their parents. Interpretative phenomenological analysis was used to analyse semi-structured interviews with eight young people (aged 14-16 years) who were the birth children of foster carers. Three superordinate themes emerged: 1. ‘relational processes that give value to my role in the family’, 2.‘threats to our relationship’ and 3.‘making sense as a way of managing the threats’. Each superordinate theme contained subthemes and whilst there were consistent patterns of experience, there was also individual variation.
The findings suggest that the processes of ‘making sense’ and ‘feeling valued’ serve to buffer the impact of potential threats to the parent-child relationship. Theoretical implications include the application of a model that has been developed to elucidate the relationship between the themes. This has clinical implications for further understanding and informing the way services support both foster carers and their children
What do we know about the impact of stress on foster carers and contributing factors?
Whilst there are increasing numbers of children in foster care, there are decreasing numbers of foster carers. Research has highlighted the many challenges that foster carers face in caring for children who have experienced adversity.
This review synthesises and evaluates the current empirical literature with the aim of exploring the causes and consequences of stress experienced by foster carers and what factors serve to lessen or increase this. PsychINFO, ASSIA, Web of Science and Google Scholar were searched for relevant studies, which were chosen for review based on specific inclusion criteria. This search identified 15 papers. Factors identified as contributing to stress included managing the impact of wider systems, such as social services and the foster carer’s family, as well as the impact of individual factors such as the child’s behaviour. Consequences of stress included a direct impact on foster carer retention. Methodological issues identified related to sampling, research design and cultural variability.
Future research could usefully include the perspectives of people in the system around foster carers, including social workers and the birth children of foster carers. Clinical implications include the promotion and provision of training and support, and the development of integrated ways of working with services and foster carers’ families
SINFONI Observations of Starclusters in Starburst Galaxies
We have used ESO's new NIR IFS SINFONI during its Science Verification period
to observe the central regions of local starburst galaxies. Being Science
Verification observations, the aim was two-fold: to demonstrate SINFONI's
capabilities while obtaining information on the nature of starclusters in
starburst galaxies. The targets chosen include a number of the brighter
clusters in NGC1808 and NGC253. Here we present first results.Comment: Submitted to "Adaptive Optics-Assisted Integral-Field Spectroscopy",
Rutten R.G.M., Benn C.R., Mendez J., eds., May 2005, La Palma (Spain), New
Astr. Re
Neutron diffraction in a model itinerant metal near a quantum critical point
Neutron diffraction measurements on single crystals of Cr1-xVx (x=0, 0.02,
0.037) show that the ordering moment and the Neel temperature are continuously
suppressed as x approaches 0.037, a proposed Quantum Critical Point (QCP). The
wave vector Q of the spin density wave (SDW) becomes more incommensurate as x
increases in accordance with the two band model. At xc=0.037 we have found
temperature dependent, resolution limited elastic scattering at 4
incommensurate wave vectors Q=(1+/-delta_1,2, 0, 0)*2pi/a, which correspond to
2 SDWs with Neel temperatures of 19 K and 300 K. Our neutron diffraction
measurements indicate that the electronic structure of Cr is robust, and that
tuning Cr to its QCP results not in the suppression of antiferromagnetism, but
instead enables new spin ordering due to novel nesting of the Fermi surface of
Cr.Comment: Submitted as a part of proceedings of LT25 (Amsterdam 2008
Quantum spin correlations in an organometallic alternating sign chain
High resolution inelastic neutron scattering is used to study excitations in
the organometallic magnet DMACuCl. The correct magnetic Hamiltonian
describing this material has been debated for many years. Combined with high
field bulk magnetization and susceptibility studies, the new results imply that
DMACuCl is a realization of the alternating
antiferromagnetic-ferromagnetic (AFM-FM) chain. Coupled-cluster calculations
are used to derive exchange parameters, showing that the AFM and FM
interactions have nearly the same strength. Analysis of the scattering
intensities shows clear evidence for inter-dimer spin correlations, in contrast
to existing results for conventional alternating chains. The results are
discussed in the context of recent ideas concerning quantum entanglement.Comment: 5 pages, 4 figures included in text. Submitted to APS Journal
Probing discs around massive young stellar objects with CO first overtone emission
We present high resolution (R~50,000) spectroastrometry over the CO 1st
overtone bandhead of a sample of seven intermediate/massive young stellar
objects. These are primarily drawn from the red MSX source (RMS) survey, a
systematic search for young massive stars which has returned a large, well
selected sample of such objects. The mean luminosity of the sample is
approximately 5 times 10^4 L_\odot, indicating the objects typically have a
mass of ~15 solar masses. We fit the observed bandhead profiles with a model of
a circumstellar disc, and find good agreement between the models and
observations for all but one object. We compare the high angular precision
(0.2-0.8 mas) spectroastrometric data to the spatial distribution of the
emitting material in the best-fitting models. No spatial signatures of discs
are detected, which is entirely consistent with the properties of the
best-fitting models. Therefore, the observations suggest that the CO bandhead
emission of massive young stellar objects originates in small-scale disks, in
agreement with previous work. This provides further evidence that massive stars
form via disc accretion, as suggested by recent simulations.Comment: Accepted for publication in MNRA
Near-infrared integral field spectroscopy of Massive Young Stellar Objects
We present medium resolution () -band integral field
spectroscopy of six MYSOs. The targets are selected from the RMS survey, and we
used the NIFS on the Gemini North telescope. The data show various spectral
line features including Br, CO, H, and \mbox{He\,{\sc i}}. The
Br line is detected in emission in all objects with
-- 200 kms. V645 Cyg shows a high-velocity
P-Cygni profile between -800 kms and -300 kms. We performed
three-dimensional spectroastrometry to diagnose the circumstellar environment
in the vicinity of the central stars using the Br line. We measured the
centroids of the velocity components with sub-mas precision. The centroids
allow us to discriminate the blueshifted and redshifted components in a roughly
east--west direction in both IRAS 18151--1208 and S106 in Br. This lies
almost perpendicular to observed larger scale outflows. We conclude, given the
widths of the lines and the orientation of the spectroastrometric signature,
that our results trace a disc wind in both IRAS 18151--1208 and S106. The CO
absorption lines at low transitions are detected in IRAS
18151--1208 and AFGL 2136. We analysed the velocity structure of the neutral
gas discs. In IRAS 18151--1208, the absorption centroids of the blueshifted and
redshifted components are separated in a direction of north-east to south-west,
nearly perpendicular to that of the larger scale jet. The
position-velocity relations of these objects can be reproduced with central
masses of 30 M_{\sun} for IRAS 18151--1208 and 20 M_{\sun} for AFGL 2136.
We also detect CO bandhead emission in IRAS 18151--1208, S106 and
V645 Cyg. The results can be fitted reasonably with a Keplerian rotation model,
with masses of 15, 20 and 20 M_{\sun} respectively.Comment: 17 pages, 10 figures, accepted by MNRA
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