Autor:
Bonifacio, P.
Caffau, E.
Spite, M.
Spite, F.
Sbordone, L.
Monaco, L.
François, P.
Plez, B.
Molaro, P.
Gallagher, A.J.
Cayrel, R.
Christlieb, N.
Klessen, R.S.
Koch, A.
Ludwig, H.-G.
Steffen, M.
Zaggia, S.
Abate, C.
Context. Extremely metal-poor (EMP) stars provide us with indirect information on the first generations of massive stars. The TOPoS survey has been designed to increase the census of these stars and to provide a chemical inventory that is as detailed as possible. Aims. Seven of the most iron-poor...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/8895
Bonifacio, P.
,
Caffau, E.
,
Spite, M.
,
Spite, F.
,
Sbordone, L.
,
Monaco, L.
,
François, P.
,
Plez, B.
,
Molaro, P.
,
Gallagher, A.J.
,
Cayrel, R.
,
Christlieb, N.
,
Klessen, R.S.
,
Koch, A.
,
Ludwig, H.-G.
,
Steffen, M.
,
Zaggia, S.
,
Abate, C.
,
[TOPoS: IV. Chemical abundances from high-resolution observations of seven extremely metal-poor stars]
,
TOPoS: IV. Chemical abundances from high-resolution observations of seven extremely metal-poor stars
