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- W66185619 abstract "I present the first results from a Hubble Space Telescope/NICMOS imaging study of the most metal-poor blue compact dwarf galaxy, I Zw 18. The near-infrared color-magnitude diagram (CMD) is dominated by two populations, one 10-20 Myr population of red supergiants and one 0.1-5 Gyr population of asymptotic giant branch stars. Stars older than 1 Gyr are required to explain the observed CMD at the adopted distance of 12.6 Mpc, showing that I Zw 18 is not a young galaxy. The results hold also if the distance to I Zw 18 is significantly larger. This rules out the possibility that I Zw 18 is a truly young galaxy formed recently in the local universe." @default.
- W66185619 created "2016-06-24" @default.
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- W66185619 date "2000-06-01" @default.
- W66185619 modified "2023-09-27" @default.
- W66185619 title "[ITAL]Hubble Space Telescope[/ITAL]/NICMOS Observations of I Z[CLC]w[/CLC] 18: A Population of Old Asymptotic Giant Branch Stars Revealed" @default.
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- W66185619 doi "https://doi.org/10.1086/312715" @default.
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