Probing population III stars in galaxy IOK-1 at z = 6.96 through He II emission
The He II λ1640 emission line has been suggested as a direct probe of Population III (PopIII) stars at high redshift, since it can arise from highly energetic ionizing photons associated with hot, metal-free stars. We use the Hubble Space Telescope WFC3/
|Collections||ANU Research Publications|
|Source:||Astrophysical Journal Letters|
|Access Rights:||Open Access|
|01_Cai_Probing_population_III_stars_2011.pdf||382.09 kB||Adobe PDF|
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