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Table 14

NGC 3766: comparison among different E(BV) estimates.

ID Other This work Sher Schild Shobbrook
Ahmed designation

1 ALS 2 398 (pe) 0.23 0.22 0.25 0.20
5 HD 306 794 0.23 ···    0.07 0.22
15 ALS 2 408 (v) 0.29 ···    0.31 0.23
24 CPD−60 3131 0.25 ···    ···    0.20
26 CPD−60 3125 (ne) 0.00 ···    0.17 ···   
27 CPD−60 3128 0.25 0.16 0.20 ···   
30 CPD−60 3135 0.07 0.18 ···    0.19
169 HD 100 969 0.27 0.18 ···    0.20
209 HD 306 800 0.37 ···    ···    0.22
232 HD 100 943* (e) 0.21 ···    0.26 0.23
239 HD 306 798 (Be) 0.37 0.19 ···    0.22
240 ALS 2 401* (Be) 0.31 ···    ···    0.19
243 HD 308 740 0.42 ···    ···    0.26
264 HD 306 657* (Be) 0.43 ···    ···    0.24
291 HD 306 793 (e) 0.34 ···    ···    0.24
301 CPD−60 3087 (e) 0.00 ···    ···    0.23
326 HD 100 840 0.28 0.21 ···    ···   

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. tars with double Balmer discontinuity. 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).

(*)

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