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Lithium in a metal-poor Halo Star
This image shows a spectrum of the metal-poor star G271-162 in the red spectral region around the Li-line at 671 nm that is used to derive the lithium isotopic ratio. The wavelengths of the doublet components of the two isotopes are indicated. The total exposure time was 3 hours and the S/N-ratio in the continuum region is above 600 - a most satisfactory result considering that the CCD fringing amplitude is more than 20% at these wavelengths.
Kredit:ESO
O snímku
Id: | eso0013b |
Typ: | Mapa |
Datum zveřejnění: | 6. dubna 2000 |
Související články: | eso0013 |
Velikost: | 800 x 602 px |
O objektu
Barvy & filtry
Pásmo | Dalekohled |
---|---|
Optický R | Very Large Telescope UVES |