Various modes of helium mixing in globular cluster giants and their possible effects on the horizontal branch morphologySUDA, Takuma; FUJIMOTO, Masayuki Y.The Astrophysical journal. 2006, Vol 643, Num 2, pp 897-916, issn 0004-637X, 20 p., 1Article

EARLY-AGE EVOLUTION OF THE MILKY WAY RELATED BY EXTREMELY METAL-POOR STARSKOMIYA, Yutaka; SUDA, Takuma; FUJIMOTO, Masayuki Y et al.The Astrophysical journal. 2009, Vol 694, Num 2, pp 1577-1594, issn 0004-637X, 18 p., 1Article

FORMATION HISTORY OF METAL-POOR HALO STARS WITH THE HIERARCHICAL MODEL AND THE EFFECT OF INTERSTELLAR MATTER ACCRETION ON THE MOST METAL-POOR STARSKOMIYA, Yutaka; HABE, Asao; SUDA, Takuma et al.The Astrophysical journal. 2010, Vol 717, Num 1, pp 542-561, issn 0004-637X, 20 p., 1Article

HIGHLY He-RICH MATTER DREDGED UP BY EXTRA MIXING THROUGH STELLAR ENCOUNTERS IN GLOBULAR CLUSTERSSUDA, Takuma; TSUJIMOTO, Takuji; SHIGEYAMA, Toshikazu et al.The Astrophysical journal. 2007, Vol 671, Num 2, issn 0004-637X, L129-L132, 2Article

The origin of carbon enhancement and the initial mass function of extremely metal-poor stars in the galactic haloKOMIYA, Yutaka; SUDA, Takuma; MINAGUCHI, Hiroki et al.The Astrophysical journal. 2007, Vol 658, Num 1, pp 367-390, issn 0004-637X, 24 p., 1Article

Is HE 0107-5240 a primordial star? The characteristics of extremely metal-poor carbon-rich starsSUDA, Takuma; AIKAWA, Masayuki; MACHIDA, Masahiro N et al.The Astrophysical journal. 2004, Vol 611, Num 1, pp 476-493, issn 0004-637X, 18 p., 1Article

Nucleosynthetic signatures of the first starsFREBEL, Anna; AOKL, Wako; HONDA, Satoshi et al.Nature (London). 2005, Vol 434, Num 7035, pp 871-873, issn 0028-0836, 3 p.Article