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Paper: The Sodium Doublets as Youth Indicators for Low-Mass Stars
Volume: 448, 16th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun
Page: 935
Authors: Schlieder, J. E.; Fielding, D.; Lepine, S.; Rice, E.; Tomasino, R.; Simon, M.; Shara, M. M.
Abstract: We investigate the use of the Na I doublets at 5890 and 5896 Å (the Fraunhofer D lines) and 8183 and 8195 Å as gravity indicators for stars of late K and M spectral type. As is well known, the equivalent widths (EWs) of these doublets increase with photospheric log(g). We show that the EWs of members of the β Pictoris moving group (BPMG) (age 10-20 Myr) lie between the EWs of giants and main sequence stars based on the analysis of approx. 200 spectra collected with the MDM 1.3-meter McGraw-Hill telescope and the SMARTS 1.5-meter telescope. We find the Na D lines are useful age indicators for low mass BPMG candidates earlier than M2 and the 8200 Å doublet becomes useful for stars later than M4. The EWs of the Na doublets may therefore be used to establish low gravity, hence youth, among low mass stars in general.
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