Published in

Cambridge University Press (CUP), Proceedings of the International Astronomical Union, S329(12), p. 69-73, 2016

DOI: 10.1017/s1743921317003301

Links

Tools

Export citation

Search in Google Scholar

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

This paper was not found in any repository, but could be made available legally by the author.
This paper was not found in any repository, but could be made available legally by the author.

Full text: Unavailable

Green circle
Preprint: archiving allowed
Green circle
Postprint: archiving allowed
Red circle
Published version: archiving forbidden
Data provided by SHERPA/RoMEO

Abstract

AbstractWe 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.

Beta version