Gaps in the Main-Sequence of Star Cluster Hertzsprung-Russell Diagrams
Priya Hasan,
Maulana Azad National Urdu University, Hyderabad, India 500032. Correspondence to: priya.hasan@gmail.com
Abstract
The presence of gaps or regions of small numbers of stars in the main sequence of the Hertzsprung-Russell Diagram (HRD) of star clusters has been reported in literature. This is interesting and significant as it could be related to star formation and/or rapid evolution or instabilities. In this paper, using Gaia DR3 photometry and confirmed membership data, we explore the HRD of nine open clusters with reported gaps, identify them and assess their importance and spectral types.
Keywords : HRD, star clusters, Gaia DR3, stellar evolution
Pour citer cet article
Priya Hasan, «Gaps in the Main-Sequence of Star Cluster Hertzsprung-Russell Diagrams», Bulletin de la Société Royale des Sciences de Liège [En ligne], Volume 93 - Année 2024, No 2 - Proceeedings of the 3rd BINA Workshop on the Scientific Potential of the Indo-Belgian Cooperation, 294-299 URL : https://popups.uliege.be/0037-9565/index.php?id=11682.