The mass-loss before the end: Two luminous blue variables with a collimated stellar wind

C. Agliozzo, C. Trigilio, C. Buemi, P. Leto, G. Umana, G. Pignata, N. M. Phillips, R. Nikutta, J. L. Prieto, J. J. Eldridge, J. C. Bray, L. A.S. McClelland, L. Xiao

Resultado de la investigación: Contribución a una revistaArtículo

Resumen

We gathered a multiwavelength dataset of two well-known LBVs. We found a complex mass-loss, with evidence of variability, such as has been seen previously. In addition, our data reveal signatures of collimated stellar winds. We propose a new scenario for these two stars where the nebula shaping is influenced by the presence of a companion star and/or fast rotation.

Idioma originalInglés
Páginas (desde-hasta)69-73
Número de páginas5
PublicaciónProceedings of the International Astronomical Union
Volumen12
N.ºS329
DOI
EstadoPublicada - 1 nov 2016

Áreas temáticas de ASJC Scopus

  • Astronomía y astrofísica

Huella Profundice en los temas de investigación de 'The mass-loss before the end: Two luminous blue variables with a collimated stellar wind'. En conjunto forman una huella única.

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    Agliozzo, C., Trigilio, C., Buemi, C., Leto, P., Umana, G., Pignata, G., Phillips, N. M., Nikutta, R., Prieto, J. L., Eldridge, J. J., Bray, J. C., McClelland, L. A. S., & Xiao, L. (2016). The mass-loss before the end: Two luminous blue variables with a collimated stellar wind. Proceedings of the International Astronomical Union, 12(S329), 69-73. https://doi.org/10.1017/S1743921317003301