Autor:
Jeffries, RD
Jackson, RJ
Franciosini, E
Randich, S
Barrado, D
Frasca, A
Klutsch, A
Lanzafame, AC
Prisinzano, L
Sacco, GG
Gilmore, G
Vallenari, A
Alfaro, EJ
Koposov, SE
Pancino, E
Bayo, A
Casey, AR
Costado, MT
Damiani, F
Hourihane, A
Lewis, J
Jofre, P
Magrini, L
Monaco, L
Morbidelli, L
Worley, CC
Zaggia, S
Zwitter, T
We show that non-magnetic models for the evolution of pre-main-sequence (PMS) stars cannot simultaneously describe the colour-magnitude diagram (CMD) and the pattern of lithium depletion seen in the cluster of young, low-mass stars surrounding gamma(2) Velorum. The age of 7.5 +/- 1 Myr inferred f...
Enlace original:
http://repositorio.unab.cl/xmlui/handle/ria/3397
Jeffries, RD
,
Jackson, RJ
,
Franciosini, E
,
Randich, S
,
Barrado, D
,
Frasca, A
,
Klutsch, A
,
Lanzafame, AC
,
Prisinzano, L
,
Sacco, GG
,
Gilmore, G
,
Vallenari, A
,
Alfaro, EJ
,
Koposov, SE
,
Pancino, E
,
Bayo, A
,
Casey, AR
,
Costado, MT
,
Damiani, F
,
Hourihane, A
,
Lewis, J
,
Jofre, P
,
Magrini, L
,
Monaco, L
,
Morbidelli, L
,
Worley, CC
,
Zaggia, S
,
Zwitter, T
,
[The Gaia-ESO Survey: lithium depletion in the Gamma Velorum cluster and inflated radii in low-mass pre-main-sequence stars]
,
The Gaia-ESO Survey: lithium depletion in the Gamma Velorum cluster and inflated radii in low-mass pre-main-sequence stars
