Results 21 to 30 of about 171,757 (316)

Broad-band spectral analysis of the accreting millisecond X-ray pulsar SAX J1748.9−2021 [PDF]

open access: yes, 2016
We analyzed a 115 ks XMM-Newton observation and the stacking of 8 days of INTEGRAL observations, taken during the raise of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1748.9-2021.
F. Pintore   +8 more
semanticscholar   +1 more source

Radio Pulse Search and X-Ray Monitoring of SAX J1808.4−3658: What Causes Its Orbital Evolution? [PDF]

open access: yes, 2016
The accreting millisecond X-ray pulsar SAX J1808.4−3658 shows a peculiar orbital evolution that proceeds at a very fast pace. It is important to identify the underlying mechanism responsible for this behavior because it can help to understand how this ...
A. Patruno   +8 more
semanticscholar   +1 more source

Knowledge mobilisation for chronic disease prevention: the case of the Australian Prevention Partnership Centre

open access: yesHealth Research Policy and Systems, 2018
Background Cross-sectoral, multidisciplinary partnership research is considered one of the most effective means of facilitating research-informed policy and practice, particularly for addressing complex problems such as chronic disease.
Sonia Wutzke   +9 more
doaj   +1 more source

Understanding the sustainment of population health programmes from a whole-of-system approach

open access: yesHealth Research Policy and Systems, 2022
Background Population health prevention programmes are needed to reduce the prevalence of chronic diseases. Nevertheless, sustaining programmes at a population level is challenging. Population health is highly influenced by social, economic and political
Melanie Crane   +5 more
doaj   +1 more source

Generalized model for anisotropic compact stars [PDF]

open access: yes, 2016
In the present investigation an exact generalized model for anisotropic compact stars of embedding class one is sought for under general relativistic background. The generic solutions are verified by exploring different physical aspects, viz.
Deb, Debabrata   +3 more
core   +2 more sources

SAX-STGCN: Dynamic Spatio-Temporal Graph Convolutional Networks for Traffic Flow Prediction

open access: yesIEEE Access, 2022
Accurate, timely, and reliable traffic flow prediction is essential for an intelligent transportation system due to the complex spatio-temporal correlation of traffic flow.
Bin Lei, Peng Zhang, Yifei Suo, Na Li
doaj   +1 more source

Beppo-SAX Observations of Galaxy Clusters [PDF]

open access: yes, 1998
The high spatial resolution of the MECS experiment on board Beppo-SAX has encouraged a few scientists, including the author, to perform observations of galaxy clusters. Results from the analysis of the first few observed objects are encouraging.
Boella   +10 more
core   +2 more sources

The SAX-3 receptor stimulates axon outgrowth and the signal sequence and transmembrane domain are critical for SAX-3 membrane localization in the PDE neuron of C. elegans.

open access: yesPLoS ONE, 2013
SAX-3, a receptor for Slit in C. elegans, is well characterized for its function in axonal development. However, the mechanism that regulates the membrane localization of SAX-3 and the role of SAX-3 in axon outgrowth are still elusive.
Jia Li, Pu Pu, Weidong Le
doaj   +1 more source

Swift monitoring of the massive X-ray binary SAX J0635.2+0533 [PDF]

open access: yes, 2017
SAX J0635.2+0533 is a binary pulsar with a very short pulsation period ($P$ = 33.8 ms) and a high long-term spin down ($\dot P$ $>$ 3.8$\times10^{-13}$ s s$^{-1}$), which suggests a rotation-powered (instead of an accretion-powered) nature for this ...
La Palombara, N., Mereghetti, S.
core   +2 more sources

THE REFLARES AND OUTBURST EVOLUTION IN THE ACCRETING MILLISECOND PULSAR SAX J1808.4–3658: A DISK TRUNCATED NEAR CO-ROTATION? [PDF]

open access: yes, 2015
The accreting millisecond X-ray pulsar SAX J1808.4–3658 shows peculiar low luminosity states known as “reflares” after the end of the main outburst. During this phase the X-ray luminosity of the source varies by up to three orders of magnitude in less ...
A. Patruno   +8 more
semanticscholar   +1 more source

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