Free Access
Table 3
Comparison of derived dust MLRs and luminosities for two C stars (TRM 88 and OGLE 051306) and two O stars.
| Reference | L | Ṁ dust | |||||
| (L⊙) | (10-9M⊙ yr-1) | ||||||
|
|
|||||||
| TRM 88 | |||||||
| van Loon et al. (1999) | 13 300 | 6.0 | |||||
| G09 | 7160 | 16.1 | |||||
| Srinivasan et al. (2011) | 11 700 | 3.4 | |||||
| Riebel et al. (2012) | 9120 ± 650 | 4.92 ± 0.58 | |||||
| present paper | 9403 | 2.1 | |||||
| OGLE 051306 | |||||||
| Srinivasan et al. (2010) | 4810, 6580 | 2.5 (2.4–2.9) | |||||
| Srinivasan et al. (2011) | 6170 | 2.4 | |||||
| Riebel et al. (2012) | 7080 ± 700 | 2.12 ± 0.42 | |||||
| present paper | 4740 | 3.2 | |||||
| HV 5715 | |||||||
| Sargent et al. (2010) | 36 000 ± 4000 | 2.3 (1.1–4.1) | |||||
| Sargent et al. (2011) | 33 000 | 1.5 | |||||
| Riebel et al. (2012) | 33 700 ± 5960 | 1.56 ± 0.43 | |||||
| Jones et al. (2012) | 28 800 | 19.6 | |||||
| Jones et al. (2014) | 19 230 ± 4300 | 0.63 ± 0.14 | |||||
| present work | 28 200 | 0.25 | |||||
| sagemcj052206 | |||||||
| Sargent et al. (2010) | 5100 ± 500 | 2.0 (1.1–3.1) | |||||
| Sargent et al. (2011) | 4900 | 2.1 | |||||
| Riebel et al. (2012) | 4820 ± 670 | 2.11 ± 0.44 | |||||
| Jones et al. (2012) | 4740 | 19.6 | |||||
| Jones et al. (2014) | 3160 ± 710 | 0.68 ± 0.19 | |||||
| present work | 4120 | 0.45 | |||||
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