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Table 13

NGC 3766: comparison among individual estimates of (mvMv)0.

ID Other This work Sher Schild Shobbrook
Ahmed designation

1 ALS 2 398 (pe) 11.97 9.27 11.10 11.71
5 HD 306 794 12.02 ···    11.80 11.36
15 ALS 2 408 (v) 11.72 ···    11.20 15.68
24 CPD−60 3131 10.54 ···    ···    11.64
26 CPD−60 3125 (ne) 11.57 ···    11.90 ···   
27 CPD−60 3128 10.28 8.99 10.80 ···   
30 CPD−60 3135 11.97 10.83 ···    11.01
169 HD 100 969 12.79 9.86 ···    11.27
209 HD 306 800 11.31 ···    ···    11.48
232 HD 100 943* (e) 13.50 ···    13.30 17.40
239 HD 306 798 (Be) 10.76 9.98 ···    11.15
240 ALS 2 401* (Be) 12.65 ···    ···    12.87
243 HD 308 740 10.91 ···    ···    10.80
291 HD 306 793 (e) 11.14 ···    ···    13.85
301 CPD−60 3087 (e) 12.47 ···    ···    13.20
326 HD 100 840 11.94 8.87 ···    ···   

Notes. (Be) Be star. (e) Emission line star. (v) Eruptive variable. (pe) Sharp Hγ line and incipient emission at Hβ. (ne) Moderate emission at Hβ. 4th column: (mvMv)0 values given by Sher (1965). 5th column: (mvMv)0 values given by Schild (1970). 6th column: (mvMv)0 values given by Shobbrook (1985).

(*)

Stars with double Balmer discontinuity.

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