They describe their required resources and simply deploy their Kubernetes clusters in any PoP on the Ridge Cloud network. Through a single API, Ericom’s developers utilize a network of service providers instead of relying on the availability of compute resources in a specific location. ImpactĮricom can now deploy applications in areas that were previously underserved by the large public clouds, with a high level of service and without issues of latency or data residency. Ericom was able to utilize the Kubernetes codebase from their existing deployments to expand their footprint without requiring any code change. This was followed by adding Points of Presence (PoPs) in Milan, Chicago, and Taipei. They began in Tel Aviv with local cloud provider MedOne, through which Ridge’s managed Kubernetes services enabled Ericom to offer solutions to local customers. Ridge enabled Ericom to deploy their zero-trust cyber security solution to new locations for which existing public cloud providers did not offer a satisfactory level of performance. SolutionĮricom reached out to CNCF partner Ridge to utilize their hybrid cloud platform which unifies application deployments across locations. Based on their need to run workloads locally and in very close proximity to end-users, Ericom realized that they would need to find a cloud with the flexibility to sit anywhere in the world where they have potential customers. Its portfolio of products features Remote Browser Isolation, which renders website content in remote containers located in the cloud and sends only safe rendering data to users’ regular web browsers. Global cybersecurity company Ericom’s solutions depend on hyper-low latency and data security. These variations also show only a weak correlation with local star formation activity within the clouds.Deploying in Any Location with Kubernetes Challenge We also find that these physical conditions and energy balance vary significantly within the Ridge and that this variation appears only weakly correlated with distance from sites of massive star formation such as R136 in 30 Dor, which is $\sim1$ kpc away. This suggests that the Ridge is not forming massive stars as actively as the other regions because it has less dense gas and not because collapse is suppressed by excess kinetic energy. We find that the Ridge has significantly lower kinetic energy at a given size scale and also lower surface densities than the other regions, resulting in higher virial parameters. We segment the emission from each region into hierarchical structures using dendrograms and analyze the sizes, masses, and linewidths of these structures. The regions 30 Dor, N159, and N113 are actively forming massive stars, while the Molecular Ridge is forming almost no massive stars, despite its large reservoir of molecular gas and proximity to N159 and 30 Dor. Finn and 11 other authors Download PDF Abstract:We present a comparison of low-J 13CO and CS observations of four different regions in the LMC - the quiescent Molecular Ridge, 30 Doradus, N159, and N113, all at a resolution of $\sim3$ pc. Download a PDF of the paper titled Structural and Dynamical Analysis of the Quiescent Molecular Ridge in the Large Magellanic Cloud, by Molly K.
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