Table 3
Elemental abundance ratios, errors in the abundance ratios, and number of lines used, for all 58 microlensed dwarf stars.
Object | ... | [Mg/Fe] | ϵ [Mg/Fe] | N(Mg) | σ(Mg) | ... |
|
||||||
. . . |
... |
. . . |
. . . |
. . . |
. . . |
... |
Notes. For each star we give abundance ratios normalised to the Sun ([X/Fe]), number of lines used for each element (N(X)), line-to-line scatter for each element (σ(X)), and the calculated uncertainty for each abundance ratio (ϵ [X/X] ). The table is only available in electronic form at the CDS.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.