Examples of using Open clusters in English and their translations into Portuguese
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Ecclesiastic
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Ecclesiastic
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Computer
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Official/political
In irregular galaxies, open clusters may be found throughout the galaxy,
It is common for two or more separate open clusters to form out of the same molecular cloud.
Other methods can then extend the distance scale from open clusters to galaxies and clusters of galaxies,
The stars formed within such a cloud compose gravitationally bound open clusters containing dozens to thousands of members with similar ages and compositions.
Young open clusters may still be contained within the molecular cloud from which they formed, illuminating it to create an H II region.
We obtained the values of the parameters, q and¿,and the values of the first q-maxwellian moments these distributions for stars of open clusters.
Morphology and classification==Open clusters range from very sparse clusters with only a few members to large agglomerations containing thousands of stars.
nebulae, and open clusters.
In irregular galaxies, open clusters may be found throughout the galaxy, although their concentration is highest where
limited only to nearby stars such as open clusters, young kinematic groups
the formation rate of open clusters is estimated to be one every few thousand years.
are called open clusters.
Galaxy clusters should not be confused with star clusters, such as open clusters, which are structures of stars within galaxies,
the RGB seen in young open clusters such as Praesepe.
In this work we study percolation on a graph for which the number of infinite open clusters presents three non-trivial phases,
are mainly observed in young cosmic structures such as open clusters, the arms of spiral galaxies,
Although there are a few hundred known open clusters within that age range,
Stellar composition==Because open clusters tend to be dispersed before most of their stars reach the end of their lives,
While open clusters and globular clusters form two fairly distinct groups,
Open clusters are not seen in elliptical galaxies:
