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Table 1:

Relevant data for our sample of S-MS stars.

Spectral type Var. type Distancea Bol. Magnitudesb Mass Loss ve Ref.c I. - E. dust/gas
Name   (GCVS) (kpc) (Paper II) (M$_{\odot}$/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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