Metallicities of Solar-type Stars in Young Open Clusters

Autor(es)

Monroe, TalaWanda R. ; Pilachowski, Catherine A. ; Rebull, Luisa ; Chavez, M ; Bertone, E ; Vega, O ; DeLaLuz, V

• Tipo de documento: Artigo Científico
• Fonte: NEW QUESTS IN STELLAR ASTROPHYSICS III: A PANCHROMATIC VIEW OF SOLAR-LIKE STARS, WITH AND WITHOUT PLANETS; v. 472, p. 2-pg., 2013-01-01.

Resumo

We present chemical abundances of six nearby young open clusters determined from moderate-resolution WIYN-Hydra and CTIO-Hydra spectra of cluster F and G pre-main sequence and main sequence stars. The selection of these particular clusters, with ages of 10-150 Myr, was aimed at examining whether the massive planet-metallicity correlation extends to younger planetary systems, namely debris disks, which are thought to be the observational signatures of planet formation. The relationship between cluster metallicity and frequency of debris disks around early-type cluster stars is explored using complementary Spitzer-MIPS 24,mu m data. Preliminary results show no strong correlation between debris disk frequency and metallicity, consistent with previous studies of older FGK stars with debris disks. (AU)

• Processo FAPESP: 10/19810-4 - Investigando a formação de planetas através de abundâncias químicas de estrelas de tipo solar
• Beneficiário: Talawanda Rose Monroe
• Modalidade de apoio: Bolsas no Brasil - Pós-Doutorado