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Home All issues Volume 499 / No 2 (May IV 2009) A&A, 499 2 (2009) 483-501 Full HTML
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Table 3:

Stellar types expected to be observable in the central parsec, considering the distance and the extinction towards the GC. Values taken from Allen's Astrophysical Quantities, the types shown here are the ones presented in that work that fall into the observational limits for the central parsec.
Early types mag K $T_{\rm eff}$ Late types $T_{\rm eff}$ mag K
B3Ia 11.80 $\sim$16 000 M6III $\sim$3200 10.78
O6I 12.12 $\sim$36 000 M4III $\sim$3400 12.32
O7V 13.92 $\sim$36 000 M2III 3540 12.92
B0V 14.65 30 000 M0III 3690 13.57
B2V 16.03 20 900 K4.5III $\sim$4100 14.29
B3V 16.33 $\sim$19 000 K2.5III $\sim$4300 15.37
B7V 17.51 $\sim$13 000 G8.5III $\sim$4750 16.42
      G7III $\sim$4900 16.50
      G5III 5050 16.62
      G4III $\sim$5100 16.77
      G0III $\sim$5200 17.27

Source LaTeX | All tables | In the text

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