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Chandra's unique ability to precisely locate and resolve individual X-ray sources in 12 globular clusters in our Galaxy has given astronomers a crucial clue as to the origin of these sources.
A surprise was that most of the star formation is in the form of star clusters — some of which survive to form the equivalent of the ancient globular clusters in our own galaxy — but most of which dissolve, their stars spreading out to form the stars that make up the galaxy as a whole.
As discussed earlier, the primary and secondary ligatures are treated as separate clusters in our study.
However, the cluster head nodes are selected by creating some clusters in our proposed algorithm.
For simplicity, we only consider closed-shell clusters in our calculations.
UPDATE: As of 1 30am CST, service has been restored to the majority of our technology clusters in our WC2 cluster.
TEM analyses revealed the presence of well-dispersed, isolated nanotubes as well as aggregated clusters in our assays.
We additionally take steps to address concerns that cluster-robust standard errors may be downwards biased, given the small number of clusters in our analysis.
None of the smaller clusters in our experiments (below 2500 µm2) exhibited synchronized network activity.
In the remaining three cases, a single MLST-defined clone was divided into two distinct clusters in our tree.
We used the map positions of the PERO markers and other Prx-based markers to assess the number of observed clusters in our data.
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