Suchergebnisse

In 2009, the Australian states and territories signed an agreement to provide 15 hours per week of universal access to quality early education to all children in Australia in the year before they enter school. Taking on board the international evidence about the importance of early education, the Commonwealth government made a considerable investment to make universal access possible by 2013. We explore the ongoing processes that seek to make universal access a reality in New South Wales by attending to the complex agential relationships between multiple actors. While we describe the state government and policy makers' actions in devising funding models to drive changes, we prioritise our gaze on the engagement of a preschool and its director with the state government's initiatives that saw them develop various funding and provision models in response. To offer accounts of their participation in policy making and doing at the preschool, we use the director's auto - biographical notes. We argue that the state's commitment to ECEC remained a form of political manoeuvring where responsibility for policy making was pushed onto early childhood actors. This manoeuvring helped to silence and further fragment the sector, but these new processes also created spaces where the sector can further struggle for recognition through the very accountability measures that the government has introduced.

SXP 1062 is a Be X-ray binary (BeXB) located in the Small Magellanic Cloud. It hosts a longperiodX- ray pulsar and is likely associated with the supernova remnant MCSNRJ0127-7332. In this work we present a multiwavelength view on SXP 1062 in different luminosity regimes. We consider monitoring campaigns in optical (OGLE survey) and X-ray (Swift telescope). During these campaigns a tight coincidence of X-ray and optical outbursts is observed. We interpret this as typical Type I outbursts as often detected in BeXBs at periastron passage of the neutron star (NS). To study different X-ray luminosity regimes in depth, during the source quiescence we observed it with XMM-Newton while Chandra observations followed an X-ray outburst. Nearly simultaneously with Chandra observations in X-rays, in optical the RSS/SALT telescope obtained spectra of SXP 1062. On the basis of our multiwavelength campaign we propose a simple scenario where the disc of the Be star is observed face-on, while the orbit of the NS is inclined with respect to the disc. According to the model of quasi-spherical settling accretion our estimation of the magnetic field of the pulsar in SXP 1062 does not require an extremely strong magnetic field at the present time.© 2018 The Author(s). ; AGG and LMO are supported by the Deutsches Zentrum fur Luft und Raumfahrt (DLR) grants FKZ 50 OR 1404 and FKZ 50 OR 1508. LMO acknowledging partial support by the Russian Government Program of Competitive Growth of Kazan Federal University. MK acknowledges funding by the Bundesministerium fur Wirtschaft und Technologie under Deutsches Zentrum fur Luft- und Raumfahrt grants 50 OR 1113 and 50 OR 1207. SBP is supported by the Russian Science Foundation grant 14-12-00146. MPES received funding through the Claude Leon Foundation Postdoctoral Fellowship program and the National Research Foundation. ; Peer Reviewed