Open Access
Table 2.
Sample of binary post-AGB stars for which the disk-mass ratio has been analyzed.
| Source | Mneb | Outflow | d | Subclass |
|---|---|---|---|---|
| [M⊙] | [%] | [pc] | ||
| AC Herculis | 8.3 × 10−4 | 5 | 1100 | Disk-dominated |
| Red Rectangle | 1.4 × 10−2 | 11 | 710 | Disk-dominated |
| IRAS 08544−4431 | 2.0 × 10−2 | ≤12 | 1100 | Disk-dominated |
| IW Carinae | 4.0 × 10−3 | ≤14 | 1000 | Disk-dominated |
| 89 Herculis | 1.8 × 10−2 | 65 | 1000 | Outflow-dominated |
| IRAS 18123+0511( * ) | 4.7 × 10−2 | 70 | 3500 | Outflow-dominated |
| IRAS 19125+0343 | 1.1 × 10−2 | 71 | 1500 | Outflow-dominated |
| R Scuti | 3.2 × 10−2 | 73 | 1000 | Outflow-dominated |
| AI Canis Minoris( * ) | 1.9 × 10−2 | 75 | 1500 | Outflow-dominated |
| IRAS 20056+1834( * ) | 1.0 × 10−1 | 75 | 3000 | Outflow-dominated |
Notes. Sources marked with an asterisk have been studied only via single-dish observations and the values of their masses and outflow-mass ratios can present higher uncertainties.
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.