Supernova Nucleosynthesis in Population III 13–50M⊙Stars and Abundance Patterns of Extremely Metal‐poor Stars
about
Massive stars. A chemical signature of first-generation very massive stars.New primary mechanisms for the synthesis of rare 9Be in early supernovae.Preserving chemical signatures of primordial star formation in the first low-mass starsThe metal and dust yields of the first massive starsThe formation of the extremely primitive star SDSS J102915+172927 relies on dustMetal enrichment in the Fermi bubbles as a probe of their origin
P2860
Supernova Nucleosynthesis in Population III 13–50M⊙Stars and Abundance Patterns of Extremely Metal‐poor Stars
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Mai 2007 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в травні 2007
@uk
name
Supernova Nucleosynthesis in P ...... of Extremely Metal‐poor Stars
@en
Supernova Nucleosynthesis in P ...... of Extremely Metal‐poor Stars
@nl
type
label
Supernova Nucleosynthesis in P ...... of Extremely Metal‐poor Stars
@en
Supernova Nucleosynthesis in P ...... of Extremely Metal‐poor Stars
@nl
prefLabel
Supernova Nucleosynthesis in P ...... of Extremely Metal‐poor Stars
@en
Supernova Nucleosynthesis in P ...... of Extremely Metal‐poor Stars
@nl
P2093
P356
P1476
Supernova Nucleosynthesis in P ...... of Extremely Metal‐poor Stars
@en
P2093
Hideyuki Umeda
Ken’ichi Nomoto
Nozomu Tominaga
P304
P356
10.1086/513063
P407
P577
2007-05-01T00:00:00Z
P5875
P818
astro-ph/0701381
P819
2007ApJ...660..516T