Results 211 to 220 of about 169,580 (246)

Soft Actuators Integrated with Control and Power Units: Approaching Wireless Autonomous Soft Robots

open access: yesAdvanced Robotics Research, EarlyView.
Soft robots exhibit significant development potential in various applications. However, there are still key technical challenges regarding material improvement, structure design and components integration. This review focuses on the development and challenge of soft actuators, power components, and control components in untethered intelligent soft ...
Renwu Shi, Feifei Pan, Xiaobin Ji
wiley   +1 more source

Age-related aberrant alternative splicing as a prognostic tool in older breast cancer patients. [PDF]

open access: yesCommun Biol
Chen M   +22 more
europepmc   +1 more source

A high-resolution atlas of the brain predicts lineage and birth order underlying neuronal identity. [PDF]

open access: yesCell Genom
Allen AM   +6 more
europepmc   +1 more source

Protocol for assembling, prioritizing, and characterizing piRNA clusters using the piRNA Cluster Builder. [PDF]

open access: yesSTAR Protoc
Ahrend F   +6 more
europepmc   +1 more source

An inflammatory and quiescent HSC subpopulation expands with age in humans. [PDF]

open access: yesGenome Biol
Safina KR   +11 more
europepmc   +1 more source

Model based clustering for young star clusters

2018
Model based clustering is a method of fitting finite mixtures models to data in order to identify clusters. It is widely used in many fields and has a variety of applications,one of those is the identification of young star clusters. We will examine four different models multivariate Gaussian, t, Skew Normal and Skew t mixtures and a method that ...
openaire   +1 more source

The Young Star Clusters in S106

1994
Near-infrared imaging of a 10 × 10 arcmin region of the S106 molecular cloud reveals two embedded clusters coinciding with peaks in the CO emission. By counting foreground stars seen towards the molecular cloud, the distance to S106 is found to be 1.2±0.2 kpc. Assuming a theoretical mass-luminosity relationship for pre-main sequence stars, we find that
openaire   +1 more source

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