Table 3
Average initial and final masses from cluster white dwarfs, based on data in Casewell et al. (2009); McDonald et al. (2011); Dobbie et al. (2012).
| Cluster | Mf | δ Mf | Mi | δ Mi |
|
|
||||
| N6819 | 0.54 | 0.01 | 1.61 | +0.1 −0.1 |
| N7789 | 0.61 | 0.02 | 2.02 | +0.1 −0.1 |
| N6791 | 0.53 | 0.01 | 1.16 | +0.1 −0.1 |
| N2168 | 0.89 | 0.02 | 4.34 | +0.2 −0.2 |
| N2516 | 0.95 | 0.02 | 5.24 | +0.5 −0.5 |
| N6633 | 0.81 | 0.05 | 3.14 | +0.2 −0.2 |
| Sirius B | 1.00 | 0.02 | 5.06 | +0.4 −0.3 |
| Praesepe | 0.76 | 0.04 | 3.37 | +0.2 −0.2 |
| Hyades | 0.69 | 0.02 | 2.75 | +0.2 −0.2 |
| Omega Cen | 0.53 | 0.03 | 0.83 | +0.05 −0.05 |
Notes. Minimum uncertainties on the initial mass are taken as 0.2 M⊙ or 0.1 M⊙ for masses of ≲ 2 M⊙ (apart for omega Cen); otherwise, the uncertainties are estimated from the scatter between individual stars in the cluster.
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.