Abstract
Luminous Blue Variables (LBV’s) are losing mass at a rate which is higher than in normal stars of the same luminosity. This high mass loss is evident from the occurrence of P Cygni profiles in the visual spectrum, the large numbers of UV lines which are Doppler shifted or show P Cygni profiles and the large IR excess or radio free-free emission. Mass loss from LBV’s is strongly variable on a wide range of timescales from months to centuries and possibly even millenia. During these variations the mass loss may vary from values as low as 10-6 to 10-5 M⊙/yr, when the star is quiet, to outbursts of the type observed in P Cygni in AD 1600 and ŋ Car in 1837 (for reviews see Davidson, 1987; Lamers, 1986, 1987).
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Lamers, H.J.G.L.M. (1989). Mass Loss from Luminous Blue Variables. In: Davidson, K., Moffat, A.F.J., Lamers, H.J.G.L.M. (eds) Physics of Luminous Blue Variables. Astrophysics and Space Science Library, vol 157. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-1031-7_17
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