Highly Enriched 7Be in the ejecta of Nova Sagittarii 2015 No. 2 (V5668 Sgr) and the Galactic Lithium origin
Paolo Molaro, Luca Izzo, Elena Mason, Piercarlo Bonifacio, Massimo, Della Valle

TL;DR
This study detects highly enriched 7Be in the ejecta of Nova Sagittarii 2015 No. 2, providing evidence that novae significantly contribute to the galactic lithium abundance through freshly synthesized 7Be during thermonuclear runaways.
Contribution
It presents the first high-resolution UV spectra detection of 7Be in a nova, showing larger amounts than current models predict and suggesting novae as major sources of galactic lithium.
Findings
Detection of 7Be in multiple high velocity components
7Be abundance much higher than predicted by models
Nova ejecta could account for all galactic lithium
Abstract
We report on the evidence of highly blue-shifted resonance lines of the singly ionised isotope of 7BeII in high resolution UVES spectra of Nova Sagittarii 2015 No. 2 (V5668 Sgr). The resonance doublet lines 7BeII at lambda 313.0583, 313.1228 nm are clearly detected in several non saturated and partially resolved high velocity components during the evolution of the outburst. The total absorption identified with Beryllium has an equivalent width much larger than all other elements and comparable to hydrogen. We estimate an atomic fraction N(7Be)/N(Ca) ~ 53-69 from unsaturated and resolved absorption components. The detection of 7Be in several high velocity components shows that it has been freshly created in a thermonuclear runaway via the reaction 3He}(alpha,gamma) 7Be during the Nova explosion, as postulated by Arnould and Norgaard (1975) , however in much larger amounts than predicted…
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