Inflows, Outflows, and a Giant Donor in the Remarkable Recurrent Nova M31N 2008-12a? - Hubble Space Telescope Photometry of the 2015 Eruption

The recurrent nova M31N 2008-12a experiences annual eruptions, contains a near-Chandrasekhar-mass white dwarf, and has the largest mass accretion rate in any nova system. In this paper, we present Hubble Space Telescope (HST) WFC3/UVIS photometry of the late decline of the 2015 eruption. We couple t...

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Detalhes bibliográficos
Autor principal: Darnley, M. J. (author)
Outros Autores: Hounsell, R. (author), Godon, P. (author), Perley, D. A. (author), Henze, M. (author), Kuin, N. P. M. (author), Williams, B. F. (author), Williams, S. C. (author), Bode, M. F. (author), Harman, D. J. (author), Hornoch, K. (author), Link, M. (author), Ness, J.-U. (author), Ribeiro, V. A. R. M. (author), Sion, E. M. (author), Shafter, A. W. (author), Shara, M. M. (author)
Formato: article
Idioma:eng
Publicado em: 2017
Assuntos:
Accretion, accretion disks
Novae, cataclysmic variables
Galaxies: individual (M31)
Stars: individual (M31N 2008-12a)
Ultraviolet: stars
Texto completo:http://hdl.handle.net/10773/18730
País:Portugal
Oai:oai:ria.ua.pt:10773/18730

Texto Completo

http://hdl.handle.net/10773/18730

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