Stellar Astrophysics
Halo stars







Accretion of gas by globular cluster stars
A. Thoul, A. Jorissen, S. Goriely, E. Jehin, P. Magain, A. Noels, and G. Parmentier
Astronomy and Astrophysics, v.383, p.491-501 (2002)
Postscript




The Self-Enrichment of Galactic Halo Globular Clusters. The mass-metallicity relation (Anglais)
G. Parmentier, G. Gilmore
Astronomy and Astrophysics, 378, 97-101 (2001)
Postscript



Field Halo Stars: the Globular Cluster Connection.
Jehin, E.; Magain, P.; Neuforge, C.; Noels, A.; Thoul, A. A.
Astronomy and Astrophysics, v.330, p.L33-L36 (1998)
Postscript




Abundance correlations in mildly metal-poor stars.
Jehin, E.; Magain, P.; Neuforge, C.; Noels, A.; Parmentier, G.; Thoul, A. A.
Astronomy and Astrophysics, v.341, p.241-255 (1999)
Postscript



The self-enrichment of galactic halo globular clusters: a clue to their formation ?
Parmentier, G.; Jehin, E.; Magain, P.; Neuforge, C.; Noels, A.; Thoul, A. A.
Astronomy and Astrophysics, v.352, p.138-148 (1999)
Postscript




The Old Halo metallicity gradient: the trace of a self-enrichment process
Parmentier, G.; Jehin, E.; Magain, P.; Noels, A.; Thoul, A. A.
Astronomy and Astrophysics, v.363, p.526-536 (2000)
Postscript




Web pages:    Sandrine Sohy
Head of research group:    Pierre Magain     Arlette Noels

Last modification: november, 22 2001.