Table 4
SED parameters.
| Star | D | L∗ | T∗ | τ10 | Rin | Reference |
| [pc] | [L⊙] | [K] | [× 1014 cm] | |||
|
|
||||||
| C stars | ||||||
| V701 Cas | 1720 | 7800 | 2800 | 0.85 | 2.1 | Menzies et al. (2006) |
| V384 Per | 560 | 8100 | 2000 | 0.25 | 2.1 | † Schöier et al. (2013) |
| GY Cam | 1030 | 7800 | 2000 | 0.3 | 2.0 | Groenewegen et al. (2002) |
| R Lep | 432 | 5500 | 2200 | 0.06 | 1.7 | † Ramstedt & Olofsson (2014) |
| V1259 Ori | 1600 | 9300 | 2200 | 1.7 | 2.2 | Menzies et al. (2006) |
| UU Aur | 260 | 6900 | 2800 | 0.017 | 1.9 | † Schöier et al. (2013) |
| V688 Mon | 1770 | 8800 | 2800 | 0.6 | 2.2 | Menzies et al. (2006) |
| AI Vol | 710 | 9000 | 2100 | 0.45 | 2.2 | † Schöier et al. (2007) |
| U Hya | 208 | *4000 | 2400 | 0.012 | 1.5 | † Ramstedt & Olofsson (2014) |
| X TrA | 360 | 5400 | 2200 | 0.024 | 1.7 | Cox et al. (2012) |
| II Lup | 500 | 8800 | 2400 | 0.55 | 2.2 | † Schöier et al. (2013) |
| V CrB | 630 | 5300 | 1800 | 0.035 | 1.7 | Cox et al. (2012) |
| V821 Her | 600 | 7900 | 2200 | 0.45 | 2.1 | † Schöier et al. (2013) |
| V Aql | 330 | 6500 | 2800 | 0.02 | 1.9 | † Schöier et al. (2013) |
| V1968 Cyg | 1480 | 10200 | 2400 | 0.85 | 2.3 | Menzies et al. (2006) |
| RV Aqr | 670 | 6800 | 2200 | 0.27 | 1.9 | † Schöier et al. (2013) |
| S stars | ||||||
| R And | 350 | 6300 | 1900 | 0.05 | 1.8 | † Ramstedt & Olofsson (2014) |
| S Cas | 570 | 8000 | 1800 | 0.5 | 2.1 | † Ramstedt & Olofsson (2014) |
| W And | 450 | 5800 | 2400 | 0.1 | 1.8 | van Leeuwen (2007) |
| R Gem | 820 | 5500 | 2400 | 0.035 | 1.7 | Whitelock et al. (2008) ‡ |
| Y Lyn | 253 | *4000 | 2400 | 0.02 | 1.5 | Ramstedt & Olofsson (2014) |
| R Cyg | 690 | 6200 | 2600 | 0.14 | 1.8 | Whitelock et al. (2008) ‡ |
| M stars | ||||||
| KU And | 680 | 11800 | 2000 | 0.90 | 2.5 | † Schöier et al. (2013) |
| AFGL 292 | 319 | *6000 | 2200 | 0.02 | 1.8 | Winters et al. (2003) |
| R Hor | 310 | 8500 | 2200 | 0.30 | 2.1 | † Schöier et al. (2013) |
| NV Aur | 1200 | 9800 | 2000 | 3.50 | 2.3 | † Schöier et al. (2013) |
| BX Cam | 500 | 7500 | 2800 | 1.30 | 2.0 | † Schöier et al. (2013) |
| GX Mon | 550 | 8200 | 2600 | 2.00 | 2.1 | † Schöier et al. (2013) |
| L2 Pup | 86 | *4000 | 2800 | 0.07 | 1.5 | Schöier et al. (2013) |
| S CMi | 470 | 5000 | 2800 | 0.07 | 1.6 | Knapp et al. (1998) |
| R LMi | 330 | 5500 | 2400 | 0.2 | 1.7 | Whitelock et al. (2008) ‡ |
| R Leo | 130 | 4600 | 1800 | 0.10 | 1.6 | † Schöier et al. (2013) |
| S CrB | 400 | 5400 | 2400 | 0.2 | 1.7 | Knapp et al. (1998) |
| V1111 Oph | 750 | 7500 | 2000 | 0.75 | 2.0 | † Schöier et al. (2013) |
| RR Aql | 530 | 7900 | 2000 | 0.70 | 2.1 | † Schöier et al. (2013) |
| V1943 Sgr | 200 | 5000 | 2200 | 0.05 | 1.6 | van Leeuwen (2007) |
| V1300 Aql | 620 | 10600 | 2000 | 3.50 | 2.4 | † Schöier et al. (2013) |
| T Cep | 190 | 5700 | 2400 | 0.10 | 1.8 | van Leeuwen (2007) |
Notes. An * indicates that the luminosity is assumed (for semi-regular variables) rather than calculated. The references listed are for distances, D, and in some cases the luminosity, L, where no period is known. A † in the references indicates that all parameters including the effective temperature, T∗, and optical depth, τ10 were also taken from the referenced DUSTY modelling. The absence of a † indicates that temperature and optical depth were calculated as part of this work. ‡ indicates that the distance was calculated from the period-magnitude relation in the cited work.
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