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The age-metallicity dependence for white dwarf stars

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The age-metallicity dependence for white dwarf stars

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Título The age-metallicity dependence for white dwarf stars
Autor Romero, Alejandra Daniela
Campos, Fabíola
Kepler, Souza Oliveira
Abstract We present a theoretical study on themetallicity dependence of the initial-to-final mass relation and its influence on white dwarf age determinations. We compute a grid of evolutionary sequences from the main sequence to ∼3000 K on the white dwarf cooling curve, passing through all intermediate stages. During the thermally pulsing asymptotic giant branch no third dredge-up episodes are considered and thus the photospheric C/O ratio is below unity for sequences with metallicities larger than Z = 0.0001. We consider initial metallicities from Z = 0.0001 to 0.04, accounting for stellar populations in the galactic disc and halo, with initial masses below ∼3M . We found a clear dependence of the shape of the initial-tofinal mass relation with the progenitor metallicity, where metal-rich progenitors result in less massive white dwarf remnants, due to an enhancement of the mass-loss rates associated with high metallicity values. By comparing our theoretical computations with semi-empirical data from globular and old open clusters, we found that the observed intrinsic mass spread can be accounted for by a set of initial-to-final mass relations characterized by different metallicity values. Also, we confirm that the lifetime spent before the white dwarf stage increases with metallicity. Finally, we estimate the mean mass at the top of the white dwarf cooling curve for three globular clusters NGC 6397, M4 and 47 Tuc, around 0.53M , characteristic of old stellar populations. However, we found different values for the progenitor mass, lower for the metal-poor cluster, NGC 6397, and larger for the younger and metal-rich cluster 47 Tuc, as expected from the metallicity dependence of the initial-to-final mass relation.
Contido em Monthly notices of the Royal Astronomical Society. Oxford. Vol. 450, no. 4 (July 2015), p. 2500–2505
Assunto Aglomerados estelares globulares
Anãs brancas
Estrelas gigantes
Evolucao estelar
[en] Stars: evolution
[en] Stars: interiors
[en] White dwarfs
Origem Estrangeiro
Tipo Artigo de periódico
URI http://hdl.handle.net/10183/126958
Arquivos Descrição Formato
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