Published in
Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S295(8), p. 322
DOI: 10.1017/s1743921313005243
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The stellar initial mass function in the early universe revealed from old stellar populations in our neighbourhood
Journal article published in 2012 by
Yutaka Komiya,
Shimako Yamada,
Takuma Suda 
,
Masayuki Y. Fujimoto
,
Masayuki Y. Fujimoto
This paper was not found in any repository, but could be made available legally by the author.
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Abstract
AbstractWe present a new method to investigate the IMF in the early universe from observations of extremely metal-poor (EMP) stars. EMP stars are the low-mass survivors of stars which are formed in the early universe. We can give constraints on the IMF from statistics of the elemental abundances of the EMP stars in the Galactic halo.