Researchers investigate chemical composition of globular cluster NGC 6362
https://phys.org/news/2017-03-chemical-composition-globular-cluster-ngc.html
European astronomers have recently studied the chemical composition of the low-mass globular cluster designated NGC 6362.
Their detailed analysis of chemical abundances for 17 elements in the cluster provides important insights into the nature
of NGC 6362. The findings were presented March 1 in a paper published online on arXiv.org.
Located about 25,000 light years away in the constellation Ara, NGC 6362 is a an irregularly shaped globular cluster. With
a mass of approximately 53,000 solar masses, it is one of the least massive globulars where multiple populations of stars
have been detected. The cluster is about 13.5 billion years old.
Although NGC 6362 is well known to astronomers, its detailed chemical composition has not been studied so far. So a team of
researchers led by Davide Massari of the Leiden Observatory in Netherlands investigated chemical abundances of this cluster.
For their study, they used the FLAMES and UVES high-resolution spectrographs mounted on the Very Large Telescope in Chile.