MUSE Observations of NGC330 in the Small Magellanic Cloud: Helium Abundance of Bright Main-sequence Stars
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-3881/ab7334/pdf
Reference98 articles.
1. Southern Hemisphere Photometry VII. The color-magnitude diagram of NGC 330 and the adjoining region of the Small Magellanic Cloud.
2. The Chemical Composition of the Sun
3. The MUSE second-generation VLT instrument
4. The effect of stellar rotation on colour-magnitude diagrams: on the apparent presence of multiple populations in intermediate age stellar clusters
5. Early disc accretion as the origin of abundance anomalies in globular clusters
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1. He abundance in NGC 1850 A and B: Are we observing the early stage of the formation of multiple populations in a stellar cluster?;Monthly Notices of the Royal Astronomical Society;2023-12-20
2. The young massive SMC cluster NGC 330 seen by MUSE;Astronomy & Astrophysics;2023-12
3. The initial spin distribution of B-type stars revealed by the split main sequences of young star clusters;Astronomy & Astrophysics;2023-02
4. Reliable stellar abundances of individual stars with the MUSE integral-field spectrograph;Monthly Notices of the Royal Astronomical Society;2022-05-24
5. The Young Massive Small Magellanic Cloud Cluster NGC 330 Observed with MUSE;Observational Imprints of Binary Evolution on B- and Be-star Populations;2022
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