| Source | Spectral type | Var. type | Distancea | Bol. Magnitudesb | Mass Loss | ve | Ref.c | I. - E. | dust/gas |
| Name | (GCVS) | (kpc) | (Paper II) | (M /yr)
|
km/s | ratio | |||
| S Cas | S3,4e-S5,8e | Mira | 0.85B | -5.71 | 1.02E-5 | 20.5 | R | I | 2.16E-4 |
| S Cas | S3,9e-S6,9e | Mira | 0.34B | -5.44 | 4.24E-6 | 17.2 | R | I | 5.66E-4 |
| S Cas | S2.5,9e-S6,9e(Tc) | Mira | 0.55B | -5.42 | 9.04E-7 | 9.0 | R | - | 1.18E-3 |
| S Cas | S6,2e-S10,4e/MSe | Mira | 0.18A | -5.39 | 8.69E-7 | 8.5 | R | I | 1.15E-4 |
| S Cas | S4,7e-S8.5,8e | Mira | 0.50B | -5.22 | 8.91E-8 | 3.8 | R | I | 6.73E-4 |
| S Cas | S2.5,5e-S6,8e: | Mira | 0.95B | -5.19 | 3.90E-7 | 7.5 | R | I | 3.70E-4 |
| S Cas | S2,9e-S8,9e(Tc) | Mira | 0.66B | -5.23 | 3.91E-7 | 4.5 | R | I | 2.67E-4 |
| S Cas | S7,8e | Mira | 0.80B | - | 7.20E-7 | 10.0 | R | I | 7.56E-4 |
| S Cas | S6,5pe | Mira | 0.97B | -5.50 | 2.26E-6 | 13.5 | R | I | 1.56E-3 |
| S Cas | S5,7e | SRB | 0.16A | -5.75 | 2.57E-6 | 14.5 | W | I | 3.71E-4 |
| S Cas | M6-7IIIaS | SRB | 0.30A | -5.64 | 1.30E-7 | 8.5 | R | I | 4.62E-3 |
| S Cas | M5-6SIIe | SRC | 0.27A | -5.63 | 4.93E-8 | 5.5 | R | I | 2.08E-3 |
| S Cas | M6SIb-II | SRC | 0.25A | -5.33 | 2.17E-7 | 7.5 | R | I | 7.83E-4 |
| S Cas | S3,5e-S8,8e/M7e | Mira | 0.41B | -5.19 | 1.09E-6 | 8.3 | R | I | 3.67E-4 |
| S Cas | S6,1e-S9,2e/M4-M1 | Mira | 0.38B | -5.27 | 2.79E-7 | 6.0 | R | I | 1.64E-3 |
| S Cas | S7,2/M6e-M7e | Mira | 0.45B | -5.44 | 1.01E-6 | 11.0 | R | I | 9.84E-4 |
| S Cas | M6eIb-II/S | SRC | 0.14A | -5.21 | 2.80E-7 | 6.8 | L | I | 6.78E-4 |
| S Cas | M5/S | LB | 0.78A | - | 3.83E-8 | 3.4 | R | I | 2.10E-2 |
| S Cas | SCe | Mira | 2.27B | -5.50 | 5.44E-6 | 13.0 | R | I | 4.41E-4 |
| S Cas | CSe | Mira | 1.39B | -5.48 | 5.17E-6 | 20.0 | R | - | 2.01E-3 |
| S Cas | C4,3e-S9,5e | Mira | 0.76B | -5.24 | 3.44E-7 | 6.0 | R | I | 1.51E-3 |
| S Cas | SC | SR | 0.69A | -6.05 | 1.70E-7 | 12.0 | R | I | 2.35E-3 |
| S Cas | C9,1p/M0ep | Mira | 1.99B | -5.87 | 3.51E-7 | 7.0 | R | I | 4.40E-3 |
Notes. (a) References for the distances are: A) the revised Hipparcos catalogue (van Leeuwen 2007); B) the period-luminosity methods for the O-rich stars as used in Paper II.
(b) Bolometric Magnitudes are taken from Paper II.
(c) References for the mass loss rates (updated
with our choice for distances) and for the outflow velocities are
quoted as: R stands for Ramstedt et al. (2009); W is for Winters et al. (2003); L for Loup et al. (1993).
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