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Table A.1

List and data for the RSGs considered by dJ88.

Object T 1 T 2 log L1 log L2 log(1) log(2) Note

TV Gem 3560 3700 4.75 4.92 −5.92 −6.46 GW
BU Gem 3440 3800 5.15 4.93 −5.68 −6.23 GW
α Ori 3500 3810 4.87 4.75 −6.02 −5.82 (1)
α Sco 3540 3550 4.74 4.85 −6.08 −6.00 (1)
RW Cyg 3365 3600 5.20 5.16 −5.30 −5.50 GW
VV Cep 3175 ... 5.13 ... −6.89 ... GW
CE Tau 3400 ... 4.55 ... −6.62 ... (4)
μ Cep 3400 3700 4.55 5.61 −5.78 −5.30 (1)
BC Cyg 3155 3575 5.54 ... −5.15 ... GW (2)
BI Cyg 3155 3575 5.38 5.09 −5.15 −5.33 GW
VY CMa 2840 3430 5.76 5.47 −3.62 −4.40 (1)
EV Car  2930 ... 5.74 5.83 −6.00 −4.90 (3)
S Per 2810 ... 5.66 4.93 −4.57 −5.16 GW
UY Sct 3000 ... 5.44 ... −5.22 ... GW
AH Sco 2800 ... 5.62 ... −6.00 ... (3)
NML Cyg 2485 3309 5.80 5.50 −4.18 −3.85 (1)

Notes. GW indicates that 1 was taken by dJ88 from Gehrz & Woolf (1971). (1) Indicates that 1 is the average of several determinations obtained with different methods. (2) BC Cyg has no IRAS fluxes at 25 and 60 μm and was not included in this study. (3) 1 from Hagen (1982). (4) 1 from Sanner (1976).

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