Nebulae around Luminous Blue Variables - large bipolar variety

Details Nebulae around Luminous Blue Variables - large bipolar variety Nebulae around Luminous Blue Variables - large bipolar variety

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..372w&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

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Stars: Variables: Other, Stars: Circumstellar Matter

Scientific paper

During the LBV phase-a short transitional phase of only the very massive stars-strong stellar winds sometimes accompanied by eruptions form small circumstellar LBV nebulae around a substantial number of LBV stars. Analyzing the morphology and and kinematics of the LBV nebulae even weakly bipolar components can be detected, leading to the conclusion that about 50% have-to some degree-a bipolar structure. A global overview of our current observational knowledge of LBV nebulae is summarized, including their morphology, sizes and kinematic parameters.

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