Eruptive Outflow Phases of Massive Stars

Details Eruptive Outflow Phases of Massive Stars Eruptive Outflow Phases of Massive Stars

2010-10-18

arxiv.org/abs/1010.3721v2

Astronomy and Astrophysics

Astrophysics

Solar and Stellar Astrophysics

10 pages. To appear in proceedings of IAU Symposium 272. Active OB Stars: structure, evolution, mass-loss, and critical limits

Scientific paper

I review recent progress on understanding eruptions of unstable massive stars, with particular attention to the diversity of observed behavior in extragalatic optical transient sources that are generally associated with giant eruptions of luminous blue variables (LBVs). These eruptions are thought to represent key mass loss episodes in the lives of massive stars. I discuss the possibility of dormant LBVs and implications for the duration of the greater LBV phase and its role in stellar evolution. These eruptive variables show a wide range of peak luminosity, decay time, expansion speeds, and progenitor luminosity, and in some cases they have been observed to suffer multiple eruptions. This broadens our view of massive star eruptions compared to prototypical sources like Eta Carinae, and provides important clues for the nature of the outbursts. I also review and discuss some implications about the possible physical mechanisms involved, although the cause of the eruptions is not yet understood.

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