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Spectrum of OGLE-TR-3
The chart displays a small portion of a high-dispersion spectrum of OGLE-TR-3, obtained with the UVES spectrograph at the 8.2-m VLT KUEYEN telescope at the Paranal Observatory (Chile). It is divided into five adjacent wavelength intervals and represents the mean of ten 1-hour spectral exposures. The fully drawn curve shows the spectrum of the "best fitting" stellar model from which the composition, temperature, mass, age of OGLE-TR-3 were deduced.
Mynd/Myndskeið:ESO
Um myndina
| Auðkenni: | eso0311b |
| Tegund: | Athuganir |
| Útgáfudagur: | 22. apríl 2003 |
| Tengdar fréttatilkynningar: | eso0311 |
| Stærð: | 2799 x 1936 px |
Um fyrirbærið
| Nafn: | OGLE-TR-3 |
| Tegund: | Milky Way : Star : Circumstellar Material : Planetary System |
| Flokkur: | Exoplanets |
