Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013)
Akito Tajitsu, Kozo Sadakane, Hiroyuki Naito, Akir Arai, and Wako Aoki

TL;DR
This study provides direct spectroscopic evidence of radioactive $^{7}$Be in a nova, indicating that classical novae can produce significant amounts of lithium, which is crucial for understanding galactic lithium evolution.
Contribution
First direct detection of radioactive $^{7}$Be in a nova, confirming nova explosions as a source of lithium in the galaxy.
Findings
Detection of $^{7}$Be in spectra 38-48 days after explosion
$^{7}$Be decays into $^{7}$Li, indicating in-situ lithium production
Supports theoretical models of lithium synthesis in novae
Abstract
The origin of lithium (Li) and its production process have long been an unsettled question in cosmology and astrophysics. Candidates environments of Li production events or sites suggested by previous studies include big bang nucleosynthesis, interactions of energetic cosmic rays with interstellar matter, evolved low mass stars, novae, and supernova explosions. Chemical evolution models and observed stellar Li abundances suggest that at least half of the present Li abundance may have been produced in red giants, asymptotic giant branch (AGB) stars, and novae. However, no direct evidence for the supply of Li from stellar objects to the Galactic medium has yet been found. Here we report on the detection of highly blue-shifted resonance lines of the singly ionized radioactive isotope of beryllium, Be, in the near ultraviolet (UV) spectra of the classical nova V339 Del (Nova Delphini…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
