Abstract
We present early high-resolution spectroscopic observations of the nova V1369 Cen. We have detected an absorption feature at 6695.6 that we have identified as blueshifted 7Li i λ6708. The absorption line, moving at -550 km s-1, was observed in five high-resolution spectra of the nova obtained at different epochs. Based on the intensity of this absorption line, we infer that a single nova outburst can inject in the Galaxy = 0.3-4.8 × 10-10 . Given the current estimates of the Galactic nova rate, this amount is sufficient to explain the puzzling origin of the overabundance of lithium observed in young star populations.
| Original language | English |
|---|---|
| Article number | L14 |
| Journal | Astrophysical Journal Letters |
| Volume | 808 |
| Issue number | 1 |
| DOIs | |
| State | Published - 20 Jul 2015 |
| Externally published | Yes |
Keywords
- Cataclysmic variables
- Galaxy: abundances
- Galaxy: evolution
- novae
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