Spectum of Be doublet
This image shows the region of the Be II doublet of the metal-poor stars LP815-43 (V = 10.91) and CD -24°17504 (V=12.18) in the reduced UVES -spectra, with Be and the other main features marked. The dotted lines are synthetic spectra computed with preliminary stellar parameters to aid the line identification. The model for LP 815-43 was computed with a tentative beryllium abundance of log(Be/H) + 12 = -1.3.
Credit:
ESO
About the Image
| Id: | eso0013a |
| Type: | Chart |
| Release date: | 6 April 2000 |
| Related releases: | eso0013 |
| Size: | 800 x 610 px |
About the Object
| Name: | CD -24°17504, LP815-43 |
| Type: | • Milky Way : Star : Type : Variable • Milky Way : Star : Spectral Type : B • X - Stars |
Colours & filters
| Band | Telescope |
| Ultraviolet U |
Very Large Telescope UVES |
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