Table 3
Typical values of Galactic ISM depletions and mean values of DLA depletions.
X | WHa | WDa | CDa | ⟨ δX ⟩ b | σXb | SEMc | δ X,medc | nc | |||||
|
|||||||||||||
Mg | 0.009 | −0.390 | −1.168 | −0.18 | 0.19 | 0.059 | −0.14 | 10 | −0.18 | 0.19 | 0.059 | −0.14 | 10 |
Si | 0.095 | −0.360 | −1.246 | −0.27 | 0.16 | 0.019 | −0.23 | 74 | −0.26 | 0.16 | 0.019 | −0.23 | 75 |
Fe | −0.592 | −1.106 | −2.108 | −0.42 | 0.28 | 0.027 | −0.39 | 105 | −0.42 | 0.28 | 0.028 | −0.39 | 106 |
Notes.
Representative values of Galactic depletions in warm-halo gas (WH), warm-disk gas (WD), and cool-disk gas (CD), calculated from Eq. (10) of Jenkins (2009) with F∗ = −0.28, 0.12, and 0.90, respectively (see Fig. 19 and Table 4 in that paper).
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.