The origin of the double main sequence in ω Centauri: Helium enrichment due to gas fueling from ITS ancient host galaxy?

Kenji Bekki*, John E. Norris

*Corresponding author for this work

    Research output: Contribution to journal › Article › peer-review

    134 Citations (Scopus)

    Fingerprint

    Dive into the research topics of 'The origin of the double main sequence in ω Centauri: Helium enrichment due to gas fueling from ITS ancient host galaxy?'. Together they form a unique fingerprint.

    Physics