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Table 2

Characteristics of RSGs for which a mass-loss rate has been measured by observing the circumstellar gas.

Name D E BV V F 60 λ m L phot 60 μm gas Method References
[kpc] [mag] [km s-1]  Jy [μm] [L] [10-6  M yr-1]
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13)

α Ori 0.130 0.18 15 299 1.64 56 000 0.15 1.5 H i  C i  K i 1 2 3
α Sco 0.185 0.10 17 115 1.73 71 000 0.12 1.0 H ii reg. 1 4 5
S Per 1.90 0.66 20 41 3.67 86 000 6.8 7.5 CO 6 6 7
PZ Cas 2.40 0.69 30 96 3.57 193 000 26 8.3 CO 8 8 7
VY CMa 1.14 0.47 47 1453 7.77 295 000 160 40 CO 9 10 11
NML Cyg 1.74 1.20 34 1030 9.80 320 000 210 140 CO 12 13 14
VX Sgr 1.57 0.52 25 263 4.14 340 000 20 11 CO 15 16 17
μ Cep 0.87 0.69 20 127 1.69 410 000 1.4 5.0 K i  Na i 6 6 18

Notes. Column (11) = reference for distance; Col. (12) = reference for E BV; Col. (13) = reference for mass-loss rate gas. The IRAS data of NML Cyg were taken from Schuster et al. (2009).

References. (1) Hipparcos parallax; (2) Lambert et al. (1984); (3) Huggins et al. (1994); (4) assumed; (5) Reimers et al. (2008); (6) LM05; (7) Woodhams (1993); (8) JB00; (9) Choi et al. (2008); (10) assuming E BV = 0.47 per kpc; (11) Decin et al. (2006) and see text; (12) Massey & Thomson (1991); (13) Blöcker et al. (2001); (14) Knapp et al. (1982); (15) Chen et al. (2007); (16) Humphreys (1978); (17) Knapp et al. (1989); (18) Guilain & Mauron (1996).

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