dc.creator | MIGUEL CHAVEZ DAGOSTINO | |
dc.date | 2011-04-01 | |
dc.date.accessioned | 2023-07-25T16:24:23Z | |
dc.date.available | 2023-07-25T16:24:23Z | |
dc.identifier | http://inaoe.repositorioinstitucional.mx/jspui/handle/1009/1814 | |
dc.identifier.uri | https://repositorioslatinoamericanos.uchile.cl/handle/2250/7807006 | |
dc.description | We analyzed the spectra of 17,600 F, G, and K stars extracted from the seventh Sloan Digital Sky Survey Data Release (SDSS-DR7) database in order to derive 〈[α/Fe]〉, [Ca/Fe], and [Mg/Fe] ratios. Particular attention has been devoted to estimating homogeneous and self-consistent atmospheric parameter values, Teƒƒ, log g, and [Fe/H], by comparing synthetic and observational Lick/SDSS indices. We present results for the sub-sample of more than 4000 spectra whose overall quality allowed us to derive fairly accurate stellar atmospheric parameter values and, therefore, reliable abundance ratios. A Monte Carlo approach was adopted to evaluate both the errors in the observational Lick/SDSS indices and in the derived parameter estimates. The analysis of the trends of [Ca/Fe] and [Mg/Fe] versus [Fe/H] pointed out that (1) the [Ca/Fe] and [Mg/Fe] ratios increase with decreasing [Fe/H] with different slopes reaching maximum average levels of +0.25 and +0.40 dex at [Fe/H]≃1.75, respectively; (2) our sample contains, at a given [Fe/H], stars characterized by significantly different amounts of α-enhancement, thus belonging to different Galactic populations; and (3) the analyzed sample shows a predominance of thick disk stars for [Fe/H] > −0.5 and the presence of stars belonging to the “high-α” halo population for −2.0 < [Fe/H] < −0.5. | |
dc.format | application/pdf | |
dc.language | eng | |
dc.publisher | The Astrophysical Journal | |
dc.relation | citation:Franchini, M., et al., (2011), THE LICK/SDSS LIBRARY. II. [Ca/Fe] AND [Mg/Fe] IN F, G, AND K STARS FROM SDSS-DR7, The Astrophysical Journal, Vol.730(117):1-13 | |
dc.rights | info:eu-repo/semantics/openAccess | |
dc.rights | http://creativecommons.org/licenses/by-nc-nd/4.0 | |
dc.subject | info:eu-repo/classification/Inspec/Galaxy: stellar content | |
dc.subject | info:eu-repo/classification/Inspec/Stars: abundances | |
dc.subject | info:eu-repo/classification/Inspec/Stars: fundamental parameters | |
dc.subject | info:eu-repo/classification/Inspec/Stars: late-type | |
dc.subject | info:eu-repo/classification/cti/1 | |
dc.subject | info:eu-repo/classification/cti/21 | |
dc.subject | info:eu-repo/classification/cti/21 | |
dc.title | THE LICK/SDSS LIBRARY. II. [Ca/Fe] AND [Mg/Fe] IN F, G, AND K STARS FROM SDSS-DR7 | |
dc.type | info:eu-repo/semantics/article | |
dc.type | info:eu-repo/semantics/acceptedVersion | |
dc.audience | students | |
dc.audience | researchers | |
dc.audience | generalPublic | |