Nuclear ashes and outflow in the eruptive star Nova Vul 1670

Tomasz Kamiński (), Karl M. Menten, Romuald Tylenda, Marcin Hajduk, Nimesh A. Patel and Alexander Kraus
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Tomasz Kamiński: European Southern Observatory, Alonso de Córdova 3107, Vitacura, Santiago, Chile
Karl M. Menten: Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
Romuald Tylenda: N. Copernicus Astronomical Center, Rabiańska 8, 87-100, Toruń, Poland
Marcin Hajduk: N. Copernicus Astronomical Center, Rabiańska 8, 87-100, Toruń, Poland
Nimesh A. Patel: Harvard-Smithsonian Center for Astrophysics, 60 Garden Street
Alexander Kraus: Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany

Nature, 2015, vol. 520, issue 7547, 322-324

Abstract: Observations of CK Vulpeculae reveal that it is surrounded by molecular gas and dust whose large mass and chemical composition cannot have come from a nova; the best explanation is that this object is the remnant of the merger of two stars.

Date: 2015
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DOI: 10.1038/nature14257

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