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Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013)

Author

Listed:
  • Akito Tajitsu

    (Subaru Telescope, National Astronomical Observatory of Japan, 650 North A'ohoku Place, Hilo, Hawaii 96720, USA)

  • Kozo Sadakane

    (Astronomical Institute, Osaka Kyoiku University, Asahigaoka, Kashiwara, Osaka 582-8582, Japan)

  • Hiroyuki Naito

    (Graduate School of Science, Nagoya University, Furo-cho, Chikusa-ku, Nagoya 464-8602, Japan
    Nayoro Observatory, 157-1 Nisshin)

  • Akira Arai

    (Center for Astronomy, University of Hyogo, Sayo-cho, Hyogo 679-5313, Japan
    Koyama Astronomical Observatory, Kyoto Sangyo University, Motoyama, Kamigamo, Kita-ku, Kyoto 603-8555, Japan)

  • Wako Aoki

    (National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka, Tokyo 181-8588, Japan)

Abstract

The origin of lithium is key to understanding the enrichment history of the Universe; now the classical nova V339 Del (Nova Delphini 2013) reveals that nova explosions could have been contributing to the recent rapid increase of the amount of lithium in the Universe.

Suggested Citation

  • Akito Tajitsu & Kozo Sadakane & Hiroyuki Naito & Akira Arai & Wako Aoki, 2015. "Explosive lithium production in the classical nova V339 Del (Nova Delphini 2013)," Nature, Nature, vol. 518(7539), pages 381-384, February.
    • Handle: RePEc:nat:nature:v:518:y:2015:i:7539:d:10.1038_nature14161
    DOI: 10.1038/nature14161
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