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The masses of globular clusters, measured by determining the dispersion in the velocities of individual stars, range from a few thousand to more than one million solar masses.
The masses of globular clusters, measured by determining the dispersion in the velocities of individual stars, range from a few thousand to more than 1,000,000 solar masses.
Main-sequence stars range from very luminous objects to faint M-type dwarf stars, and they vary considerably in their surface temperatures, their bolometric (total) luminosities, and their radii.
These stars range from hot, O- and B-type, blue objects at least 10,000 times brighter than the Sun down through white A-type stars such as Sirius to orange K-type stars such as Epsilon Eridani and finally to M-type red dwarfs thousands of times fainter than the Sun.
The estimated mass loss rates show a decreasing trend with time, except for very young stars, thought there is still a large scatter in the data, partly because the observed stars range from very low-mass to near solar-mass stars 1 1.
"Although their exact ages remain uncertain, astronomers estimate that NGC 2547's stars range from 20 to 35 million years old," officials from the ESO wrote in a statement.
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