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Empirical effective temperatures of late O, B, A and early F stars
Empirical effective temperatures of 99 late O, B, A and early F starshave been derived by combining space observations in the ultravioletwith ground-based observations and by fitting the computed fluxes to theobserved fluxes in the visible and ultraviolet spectral ranges.Effective temperatures found here are in good agreement with thosederived by previous workers.
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Gözlemler ve gökölçümü verileri
| Takýmyýldýz: | Anka |
| Sað Açýklýk: | 00h12m29.83s |
| Yükselim: | -56°24'48.0" |
| Görünürdeki Parlaklýk: | 9.855 |
| özdevim Sað Açýklýk: | 13.7 |
| özdevim Yükselim: | -6.7 |
| B-T magnitude: | 10.472 |
| V-T magnitude: | 9.906 |
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