Table 4
Galactic extreme carbon stars.
| Identifier | Other name | Period | Amp. (Fil.) | Ref. | v exp | Lum. | d | MLRDUSTY | v exp,DUSTY | r gd | MLRscaled |
| (days) | (mag) | (km s-1) | (L⊙) | (kpc) | (10-5M⊙ yr-1) | (km s-1) | (10-5M⊙ yr-1) | ||||
|
|
|||||||||||
| AFGL 190 | 01144+6658 | 1060 | 1.2 (L) | 1 | 18.0 | 16 400 | 3.30 | 5.7 | 10.5 | 67 | 3.3 |
| AFGL 341 | 02293+5748 | 815 | 0.9 (L) | 1 | 14.2 | 12 500 | 2.81 | 2.6 | 14.2 | 199 | 2.6 |
| IRAS 03448+4432 | AFGL 5102 | 729 | 0.7 (K) | 2 | 13.3 | 11 100 | 2.31 | 1.4 | 20.6 | 477 | 2.2 |
| AFGL 865 | 06012+0726 | 696 | 0.9 (K) | 3 | 16.6 | 10 600 | 1.72 | 1.5 | 17.9 | 234 | 1.6 |
| IRAS 08074-3615 | V688 Pup | 832 | 0.9 (K) | 4 | 21.7 | 12 700 | 2.95 | 2.0 | 19.2 | 156 | 1.7 |
| AFGL 2494 | 19594+4047 | 783 | 1.0 (L) | 5 | 20.5 | 12 000 | 1.50 | 1.4 | 20.0 | 191 | 1.3 |
| AFGL 3068 | 23166+1655 | 696 | 0.9 (K) | 3 | 15.1 | 10 600 | 1.05 | 3.9 | 13.9 | 168 | 3.6 |
Reference. For the pulsation periods and semi-amplitudes are (1) Groenewegen et al. (1998), based on L-band data from R. R. Joyce (1996, priv. comm.); (2) Kerschbaum et al. (2006); (3) Le Bertre (1992); (4) Whitelock et al. (2006); and (5) Jones et al. (1990). The output from MoD for the gas MLR and expansion velocity scale with (rgd/ 200)p with power p = 0.5 and − 0.5, respectively.
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