Multiwavelength observations of nova SMCN 2016-10a - one of the brightest novae ever observed

We report on multiwavelength observations of nova Small Magellanic Cloud Nova 2016-10a. The present observational set is one of the most comprehensive for any nova in the Small Magellanic Cloud, including low-, medium-, and high-resolution optical spectroscopy and spectropolarimetry from Southern Af...

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Detalhes bibliográficos
Autor principal: Aydi, E. (author)
Outros Autores: Page, K. L. (author), Kuin, N. P. M. (author), Darnley, M. J. (author), Walter, F. M. (author), Mróz, P. (author), Buckley, D. (author), Mohamed, S. (author), Whitelock, P. (author), Woudt, P. (author), Williams, S. C. (author), Orio, M. (author), Williams, R. E. (author), Beardmore, A. P. (author), Osborne, J. P. (author), Kniazev, A. (author), Ribeiro, V. A. R. M. (author), Udalski, A. (author), Strader, J. (author), Chomiuk, L. (author)
Formato: article
Idioma:eng
Publicado em: 2018
Assuntos:
stars: individual (SMCN 2016-10a)
novae, cataclysmic variables
white dwarfs
ultraviolet: stars
X-rays: binaries
Texto completo:http://hdl.handle.net/10773/21416
País:Portugal
Oai:oai:ria.ua.pt:10773/21416

Texto Completo

http://hdl.handle.net/10773/21416

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