Table 2
Parameters of best-fitting models for all sources in our database.
| id | RA (J2000) | Dec (J2000) | τ0.55 | log Ṁ/M⊙ | L/L⊙ | Class | Flag | |||||||
|
|
||||||||||||||
| 1 | 05:02:00.86 | −65:23:12.3 | 0.000 | –99.999 | 3263 | O | U | |||||||
| 2 | 05:02:01.65 | −66:16:00.2 | 0.000 | –99.999 | 4847 | O | U | |||||||
| 3 | 05:02:02.88 | −66:46:51.6 | 0.137 | –7.462 | 5645 | C | S | |||||||
| 4 | 05:02:07.10 | −66:56:03.1 | 0.019 | –8.596 | 5402 | O | S | |||||||
| 5 | 05:02:09.01 | −66:18:57.2 | 0.340 | –7.069 | 5544 | C | S | |||||||
Notes. Only the first entries are shown here as an example. The full table is available at the CDS. The fourth column is the optical depth at 0.55 μm. For stars without a dusty envelope, the logarithm of the mass-loss rate (5th column), was set to − 99.999. The 7th column indicates the C- and O-rich classification. Sources flagged “B” indicate stars with bad fits while “U” stands for uncertain classification and “S” for secure classification.
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