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Table 4

Effective temperature estimations for R 40 and R 110, based on different spectroscopic and photometric criteria, where >A2 corresponds to spectral types later than A2.

Year Mg II 4482 Å/He I 4471 Å Spectral Spectral Teff (K)1 Teff (K)2 Teff (K)3
type1 type HM84 EH03
R 40

1960 B8Ieq4 10 900 12 000
1960 −0.034 11 100
1966 −0.015 10 500
1968 −0.046 11 400
1974 −0.017 10 500
1983 0.018 10 000
1991 0.059 9200
1994 A49 8800 8000
2002 4.70 ± 1.14 A2 8500
2005 3.77 ± 0.73 A0–A2 9000
2005 A0 ~A2 9300 9000
2006 5.40 ± 1.38 ~A2 8500
2007 7.00 ± 2.29 >A2 <8500
2008 6.50 ± 0.94 >A2 <8500
2014 0.48 6200
2015 0.51 6100
2016 F8Iab 6200 5750
June/2016 0.57 5900
December/2016 0.65 5800

R 110

1960 B9Ieq4 10 250 10 500
1969 0.0410 9400
1982 0.048 9400
1984 0.068 9000
1989 0.158 7800
1989 F0Ia8 7800 6750
2005 B9 10 250 10 500
2005 1.95 ± 0.34 B9 10 500
2007 2.69 ± 0.63 A0–A2 9000
2014 3.54 ± 0.89 A0–A2 9000
2014 A0–A2 9300 9000
2014 0.0311 9600
2016 5.00 ± 1.70 A2 8500
2016 A2 9100 8500
2016 0.03 9600

Notes. (1) Spectral type and Teff were estimated from Mg II 4482 Å/He I 4471 Å ratio; these measurements were only obtained for spectra for which the lines are not blended; (2) Teff was estimated using the relation for spectral types from Humphreys & McElroy (1984, Table 2) (HM84) and Evans & Howarth (2003, Table 5) (EH03); and (3) Teff was estimated from . Owing to the uncertainty in the reddening, the error is K for Teff ≥ 9000 K and K for Teff < 9000 K. The references are (4) Feast et al. (1960), (5) Butler (1972), (6) Dachs (1970), (7) Ardeberg & Maurice (1977), (8) Stahl et al. (1985), (9) Szeifert et al. (1993), (10) Mendoza (1970), and (11) AAVSO. The other values are from this work.

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