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WebThese young clusters have several designations: young populous clusters, blue globular clusters and young globular clusters. We will concentrate here on the brightest examples, such as NGC 1831, 1866, 2164, 2214 and the 30-Dor cluster. In mass and binding energy, they are like average globular clusters in the Galaxy: their masses are typically ... Web8 nov. 2009 · Most of these clusters are confined to a narrow age range centred around 10 Myr because of observational constraints. At this age, the cluster light is dominated by … highest a1c reported
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Webcluster dynamics (Section 3) and the binary contributions in star clusters as a function of age (Section 4). In Section 5, I will conclude this contribution by highlighting some of the remaining uncertainties hampering a more detailed understanding of the underlying physics driving star cluster evolution and its observational interpretation. 2. Web17 feb. 2024 · Steven N. Shore, in Encyclopedia of Physical Science and Technology (Third Edition), 2003 IV.H Variable Stars. The primary variable stars in these clusters are the RR Lyrae type, which have periods of about 0.3–0.6 day. Originally called cluster variables, they have been extensively cataloged in the past several decades. The light curves fall … WebIt is dominated by young, blue Population I stars. The central bulge is devoid of gas and dust. As you might expect, the bulge is composed primarily of Population II stars. Type c spiral galaxies have the most gas and dust. Lenticular Galaxies M85 Courtesy of The Digitized Sky Survey highest aav in baseball