The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
about
The U/Th production ratio and the age of the Milky Way from meteorites and Galactic halo stars.Nucleosynthesis in neutron-rich ejecta from quark-novaePrincipal component analysis on chemical abundances spacesSilver and palladium help unveil the nature of a second r-processHeavy element synthesis in the oldest stars and the early Universe
P2860
The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
description
2002 nî lūn-bûn
@nan
2002 թուականի Յունիսին հրատարակուած գիտական յօդուած
@hyw
2002 թվականի հունիսին հրատարակված գիտական հոդված
@hy
2002年の論文
@ja
2002年論文
@yue
2002年論文
@zh-hant
2002年論文
@zh-hk
2002年論文
@zh-mo
2002年論文
@zh-tw
2002年论文
@wuu
name
The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
@ast
The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
@en
type
label
The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
@ast
The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
@en
prefLabel
The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
@ast
The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
@en
P2093
P356
P1476
The Chemical Composition and Age of the Metal‐poor Halo Star BD +17o3248
@en
P2093
Bernd Pfeiffer
Christopher Sneden
Francesca Primas
George M. Fuller
Inese I. Ivans
James E. Lawler
James W. Truran
John J. Cowan
Karl‐Ludwig Kratz
Scott Burles
P304
P356
10.1086/340347
P407
P577
2002-06-20T00:00:00Z
P5875
P818
astro-ph/0202429
P819
2002ApJ...572..861C