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

Kenji Bekki, J. E. Norris

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

134 Citations (Scopus)

Original language	English
Pages (from-to)	L109-L112
Journal	The Astrophysical Journal
Volume	2006 February 1
Issue number	637
DOIs	https://doi.org/10.1086/500413
Publication status	Published - 2006

Access to Document

10.1086/500413

Cite this

@article{c5ba73ec85d241a48e5b7ad1587b5019,

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

author = "Kenji Bekki and Norris, {J. E.}",

year = "2006",

doi = "10.1086/500413",

language = "English",

volume = "2006 February 1",

pages = "L109--L112",

journal = "The Astrophysical Journal",

issn = "0004-637X",

publisher = "IOP Publishing",

number = "637",

}

TY - JOUR

T1 - The origin of the double main sequence in ω Centauri: Helium enrichment due to gas fueling from ITS ancient host galaxy?

AU - Bekki, Kenji

AU - Norris, J. E.

PY - 2006

Y1 - 2006

U2 - 10.1086/500413

DO - 10.1086/500413

M3 - Article

SN - 0004-637X

VL - 2006 February 1

SP - L109-L112

JO - The Astrophysical Journal

JF - The Astrophysical Journal

IS - 637

ER -