Initial fractional abundances f0(X)a of parent species, relative to H2, for the O-rich AGB star, IK Tau.
|4||N2||1.5(–4)||Shock-induced non-LTE abundancee|
|7||CO2||4.4(–9)||Shock-induced non-LTE abundancee|
|13||H2S||1.0(–8)||Shock-induced non-LTE abundancee|
|14||HS||2.3(–8)||Shock-induced non-LTE abundancee|
|17||HCl||3.7(–7)||Shock-induced non-LTE abundancee|
Notes. a(b) = a × 10b.
See Table 6 in Decin et al. (2010b). In that work the fractional abundance was given relative to the total H-content, nH, by assuming all hydrogen is in its molecular form, H2, i.e., nH = 2n(H2).
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.