Table B1.

The mechanical luminosities of 25 O stars in LH 90.

IDaSp-typea|$M_{\rm bol}^a$||$\lg T_*^a$||$v_w^b$||$\lg \dot {M}$|Lw
(mag)(km s−1)(1036 erg s−1)
2–01O5.5 III−9.734.622000−5.712.49
2–02O7:−8.074.602400−6.680.38
2–03O5.5 V−9.614.642000−5.752.26
2–04O8 V−7.434.581900−6.940.13
2–08O9.7 I−10.634.481700−4.8525.89
2–10O3-6−7.764.652900−6.880.35
2–11O9 V−7.394.551500−6.890.09
2–13O6: f−9.214.602300−6.061.46
2–14O5.5 III−7.864.622000−6.690.26
2–16O8 V−7.264.581900−7.030.11
2–17O8 V−7.984.581900−6.650.26
2–20O5.5 III−8.954.622000−6.120.97
2–22O3 III(f*)−9.914.673000−5.745.22
2–24O6 V−8.094.632600−6.680.45
2–26O9 V−7.224.551500−6.980.08
2–28O8 V−8.544.581900−6.350.51
2–29O9:−8.214.531500−6.470.24
2–30O7:−9.414.582400−6.001.85
2–32O6: I−9.414.582300−5.5010.71
2–33O5.5 III−9.254.622000−5.961.39
2–36O8 V−9.134.581900−6.041.04
2–38AO9-B0−9.344.481500−5.930.84
2–50O7 III−8.964.582600−6.271.16
2–51O7 V−8.204.602400−6.610.45
2–53O6 If−10.334.582300−5.0331.13
Total89.71
IDaSp-typea|$M_{\rm bol}^a$||$\lg T_*^a$||$v_w^b$||$\lg \dot {M}$|Lw
(mag)(km s−1)(1036 erg s−1)
2–01O5.5 III−9.734.622000−5.712.49
2–02O7:−8.074.602400−6.680.38
2–03O5.5 V−9.614.642000−5.752.26
2–04O8 V−7.434.581900−6.940.13
2–08O9.7 I−10.634.481700−4.8525.89
2–10O3-6−7.764.652900−6.880.35
2–11O9 V−7.394.551500−6.890.09
2–13O6: f−9.214.602300−6.061.46
2–14O5.5 III−7.864.622000−6.690.26
2–16O8 V−7.264.581900−7.030.11
2–17O8 V−7.984.581900−6.650.26
2–20O5.5 III−8.954.622000−6.120.97
2–22O3 III(f*)−9.914.673000−5.745.22
2–24O6 V−8.094.632600−6.680.45
2–26O9 V−7.224.551500−6.980.08
2–28O8 V−8.544.581900−6.350.51
2–29O9:−8.214.531500−6.470.24
2–30O7:−9.414.582400−6.001.85
2–32O6: I−9.414.582300−5.5010.71
2–33O5.5 III−9.254.622000−5.961.39
2–36O8 V−9.134.581900−6.041.04
2–38AO9-B0−9.344.481500−5.930.84
2–50O7 III−8.964.582600−6.271.16
2–51O7 V−8.204.602400−6.610.45
2–53O6 If−10.334.582300−5.0331.13
Total89.71

Notes. The units of T and |$\dot {M}$| are K and M yr−1, respectively. This result requires a further correction for low metallicity in the LMC.

Reference: aTestor et al. (1993); bKudritzki & Puls (2000).

Table B1.

The mechanical luminosities of 25 O stars in LH 90.

IDaSp-typea|$M_{\rm bol}^a$||$\lg T_*^a$||$v_w^b$||$\lg \dot {M}$|Lw
(mag)(km s−1)(1036 erg s−1)
2–01O5.5 III−9.734.622000−5.712.49
2–02O7:−8.074.602400−6.680.38
2–03O5.5 V−9.614.642000−5.752.26
2–04O8 V−7.434.581900−6.940.13
2–08O9.7 I−10.634.481700−4.8525.89
2–10O3-6−7.764.652900−6.880.35
2–11O9 V−7.394.551500−6.890.09
2–13O6: f−9.214.602300−6.061.46
2–14O5.5 III−7.864.622000−6.690.26
2–16O8 V−7.264.581900−7.030.11
2–17O8 V−7.984.581900−6.650.26
2–20O5.5 III−8.954.622000−6.120.97
2–22O3 III(f*)−9.914.673000−5.745.22
2–24O6 V−8.094.632600−6.680.45
2–26O9 V−7.224.551500−6.980.08
2–28O8 V−8.544.581900−6.350.51
2–29O9:−8.214.531500−6.470.24
2–30O7:−9.414.582400−6.001.85
2–32O6: I−9.414.582300−5.5010.71
2–33O5.5 III−9.254.622000−5.961.39
2–36O8 V−9.134.581900−6.041.04
2–38AO9-B0−9.344.481500−5.930.84
2–50O7 III−8.964.582600−6.271.16
2–51O7 V−8.204.602400−6.610.45
2–53O6 If−10.334.582300−5.0331.13
Total89.71
IDaSp-typea|$M_{\rm bol}^a$||$\lg T_*^a$||$v_w^b$||$\lg \dot {M}$|Lw
(mag)(km s−1)(1036 erg s−1)
2–01O5.5 III−9.734.622000−5.712.49
2–02O7:−8.074.602400−6.680.38
2–03O5.5 V−9.614.642000−5.752.26
2–04O8 V−7.434.581900−6.940.13
2–08O9.7 I−10.634.481700−4.8525.89
2–10O3-6−7.764.652900−6.880.35
2–11O9 V−7.394.551500−6.890.09
2–13O6: f−9.214.602300−6.061.46
2–14O5.5 III−7.864.622000−6.690.26
2–16O8 V−7.264.581900−7.030.11
2–17O8 V−7.984.581900−6.650.26
2–20O5.5 III−8.954.622000−6.120.97
2–22O3 III(f*)−9.914.673000−5.745.22
2–24O6 V−8.094.632600−6.680.45
2–26O9 V−7.224.551500−6.980.08
2–28O8 V−8.544.581900−6.350.51
2–29O9:−8.214.531500−6.470.24
2–30O7:−9.414.582400−6.001.85
2–32O6: I−9.414.582300−5.5010.71
2–33O5.5 III−9.254.622000−5.961.39
2–36O8 V−9.134.581900−6.041.04
2–38AO9-B0−9.344.481500−5.930.84
2–50O7 III−8.964.582600−6.271.16
2–51O7 V−8.204.602400−6.610.45
2–53O6 If−10.334.582300−5.0331.13
Total89.71

Notes. The units of T and |$\dot {M}$| are K and M yr−1, respectively. This result requires a further correction for low metallicity in the LMC.

Reference: aTestor et al. (1993); bKudritzki & Puls (2000).

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