Table 1.
Physical and dust properties of the LMC and SMC sources classified as shell-type post AGB stars by K14 and K15.
| ID | [Fe/H] | Teff[K] | L/L⊙ | τ10 | Td[K] | Rin/R⊙ | M/M⊙ |
|---|---|---|---|---|---|---|---|
| J052220.98 | −0.50 | 5750 | 4500 | 0.015 | 220 | 2.63 × 105 | 0.9 |
| J053250.69 | −1.10 | 6000 | 5200 | 0.006 | 250 | 2.06 × 105 | 1.00 |
| J004114.10 | −1.04 | 5750 | 5800 | 0.007 | 280 | 1.65 × 105 | 1.00 |
| J050632.10 | −0.40 | 7600 | 6000 | 0.003 | 240 | 2.74 × 105 | 1.25 |
| J003643.94 | −0.63 | 7500 | 6500 | 0.002 | 250 | 2.56 × 105 | 1.50 |
| J051848.84 | −1.00 | 6000 | 6700 | 0.008 | 240 | 2.62 × 105 | 1.25 |
| J004441.03 | −1.07 | 6000 | 8500 | 0.002 | 320 | 6.64 × 104 | 2.00 |
| J005803.08 | −1.03 | 6500 | 12000 | 0.025 | 280 | 1.20 × 105 | 2.50 |
| J045119.94 | −0.40 | 8250 | 5000 | 0.006 | 270 | 2.97 × 104 | 0.80 |
| J052241.52 | −0.50 | 8250 | 5000 | 0.017 | 400 | 2.26 × 104 | 0.80 |
| J052740.75 | −0.50 | 8250 | 5200 | 0.024 | 470 | 1.22 × 104 | 0.90 |
| J050221.17 | −0.60 | 5250 | 4500 | 0.022 | 180 | 5.45 × 104 | 0.80 |
| J051906.86 | −1.30 | 5500 | 3800 | 0.015 | 180 | 5.13 × 104 | 0.65 |
Notes. The quantities listed in the various columns are the following: 1: Source ID; 2, 3: Metallicity and effective temperature derived spectroscopically by K14 and K15; 4–7: Luminosity, optical depth at 10 μm, dust temperature, and distance separating the central star from the inner border of the dusty region, found via SED fitting; 8: Mass of the progenitor at the beginning of the AGB phase, deduced via comparison of the derived luminosity with results from post-AGB evolution modelling.
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.