Table 12
NGC 3766: comparison among different Mv estimates.
ID | Other | This work | Sher | Balona | Shobbrook |
Ahmed | designation | ||||
|
|||||
1 | ALS 2 398 (pe) | −4.05 | −1.26 | −2.00 | −3.75 |
5 | HD 306 794 | −4.56 | ··· | −3.70 | −3.88 |
15 | ALS 2 408 (v) | −4.09 | ··· | −2.60 | −7.87 |
24 | CPD−60 3131 | −0.02 | ··· | −1.30 | −1.01 |
26 | CPD−60 3125 (ne) | −2.51 | ··· | −3.10 | ··· |
27 | CPD−60 3128 | −2.58 | −1.10 | −3.10 | ··· |
30 | CPD−60 3135 | −1.08 | −0.30 | −1.60 | −0.53 |
55 | CPD−60 3138 | −0.54 | ··· | −1.00 | ··· |
97 | CPD−60 3098 | −2.59 | ··· | −2.60 | ··· |
151 | CD−60 3626 | −1.56 | ··· | −2.00 | ··· |
169 | HD 100 969 | −4.60 | −1.26 | −4.50 | −2.75 |
209 | HD 306 800 | −1.65 | ··· | −2.00 | −1.52 |
232 | HD 100 943* (e) | −7.00B | ··· | −7.00 | −10.95 |
239 | HD 306 798 (Be) | −2.53 | −1.10 | −2.60 | −2.37 |
240 | ALS 2 401* (Be) | −4.01 | ··· | −3.60 | −3.84 |
243 | HD 308 740 | −1.11 | ··· | −1.30 | −0.66 |
264 | HD 306 657* (Be) | −2.62 | ··· | −2.50 | ··· |
291 | HD 306 793 (e) | −1.53 | ··· | −2.00 | −3.94 |
301 | CPD−60 3087 (e) | −1.57 | ··· | −2.00 | −3.08 |
316 | BF Cen (A) | −3.60 | ··· | −3.70 | ··· |
317 | HD 306 785 | −2.59 | ··· | −3.70 | ··· |
326 | HD 100 840 | −4.61 | −1.26 | −3.90 | ··· |
··· | HD 306 644 | −2.10 | ··· | −1.70 | ··· |
··· | HD 306 778 | −2.10 | ··· | −2.00 | ··· |
··· | HD 306 784 | −0.01 | ··· | −1.00 | ··· |
··· | HD 306 787 | −1.06 | ··· | −1.30 | ··· |
··· | HD 306 788 | −2.06 | ··· | −2.00 | ··· |
··· | HD 308 743 | −1.52 | ··· | −2.00 | ··· |
··· | HD 308 852 * | −1.54 | ··· | −1.80 | ··· |
··· | NGC 3766 MG 29 | −1.58 | ··· | −2.00 | ··· |
··· | NGC 3766 MG 116 | −1.10 | ··· | −1.30 | ··· |
··· | NGC 3766 MG 177 | −2.53 | ··· | −2.60 | ··· |
Notes. (A) Algol eclipsing binary. (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: Mv values given by Sher (1965). 5th column: Mv values given by Balona & Crampton (1974). 6th column: Mv values given by Shobbrook (1985).
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