Lithium in M 67: From the main sequence to the red giant branch


Autoria(s): Pace, G.; Castro, M.; Melendez, J.; Theado, S.; Nascimento Jr., J. D. do
Contribuinte(s)

UNIVERSIDADE DE SÃO PAULO

Data(s)

24/09/2013

24/09/2013

01/05/2012

Resumo

Context. Lithium abundances in open clusters are a very effective probe of mixing processes, and their study can help us to understand the large depletion of lithium that occurs in the Sun. Owing to its age and metallicity, the open cluster M 67 is especially interesting on this respect. Many studies of lithium abundances in M 67 have been performed, but a homogeneous global analysis of lithium in stars from subsolar masses and extending to the most massive members, has yet to be accomplished for a large sample based on high-quality spectra. Aims. We test our non-standard models, which were calibrated using the Sun with observational data. Methods. We collect literature data to analyze, for the first time in a homogeneous way, the non-local thermal equilibrium lithium abundances of all observed single stars in M 67 more massive than similar to 0.9 M-circle dot. Our grid of evolutionary models is computed assuming a non-standard mixing at metallicity [Fe/H] = 0.01, using the Toulouse-Geneva evolution code. Our analysis starts from the entrance into the zero-age main-sequence. Results. Lithium in M 67 is a tight function of mass for stars more massive than the Sun, apart from a few outliers. A plateau in lithium abundances is observed for turn-off stars. Both less massive (M >= 1.10 M-circle dot) and more massive (M >= 1.28 M-circle dot) stars are more depleted than those in the plateau. There is a significant scatter in lithium abundances for any given mass M <= 1.1 M-circle dot. Conclusions. Our models qualitatively reproduce most of the features described above, although the predicted depletion of lithium is 0.45 dex smaller than observed for masses in the plateau region, i.e. between 1.1 and 1.28 solar masses. More work is clearly needed to accurately reproduce the observations. Despite hints that chromospheric activity and rotation play a role in lithium depletion, no firm conclusion can be drawn with the presently available data.

FCT/CAPES

FCT/CAPES [237/09]

Fundacao para a Ciencia e Tecnologia (FCT), Portugal

Fundacao para a Ciencia e a Tecnologia (FCT), Portugal

CNPq Brazilian Agency

Brazilian agency CNPq

FAPERN Brazilian Agency

FAPERN Brazilian Agency

USP, FAPESP [2010/17510-3]

USP, FAPESP

CNPq (Bolsa de Produtividade)

CNPq (Bolsa de Produtividade)

[SFRH/BPD/39254/2007]

[PTDC/CTE-AST/098528/2008]

Identificador

ASTRONOMY & ASTROPHYSICS, LES ULIS CEDEX A, v. 541, MAY, 2012

0004-6361

http://www.producao.usp.br/handle/BDPI/33625

10.1051/0004-6361/201117704

http://dx.doi.org/10.1051/0004-6361/201117704

Idioma(s)

eng

Publicador

EDP SCIENCES S A

LES ULIS CEDEX A

Relação

Astronomy and Astrophysics

Direitos

openAccess

Copyright EDP SCIENCES S A

Palavras-Chave #STARS: ABUNDANCES #STARS: ATMOSPHERES #SOLAR-TYPE STARS #STELLAR RADIATIVE ZONES #LOW-MASS STARS #CHROMOSPHERIC ACTIVITY #OPEN CLUSTER #INTERNAL WAVES #CHEMICAL-COMPOSITION #EVOLUTIONARY MODELS #ELEMENT ABUNDANCES #INTERMEDIATE-AGE #ASTRONOMY & ASTROPHYSICS
Tipo

article

original article

publishedVersion