Abstract
AG Car is one of the few Luminous Blue Variables (LBV’s) in our galaxy. The star is a photometric variable which had a recent outburst in 1981 (Whitelock et al., 1983; Wolf and Stahl, 1982) and is surrounded by a resolved ring nebula (Thackeray, 1950; Paresce, 1989). These properties indicate that AG Car is a typical LBV. However, at its canonical distance of 2-2.5 kpc, derived from its assumed membership of the Car OBI or OB2 association, AG Car has a bolometric luminosity of M bol -8.5 to -9.0 and is located significantly below the Humphreys-Davidson limit, and also below the upperlimit for red supergiants (RSG). This implies that AG Car might have been a RSG and that the ring might be due to the interaction of the RSG wind and the LBV wind.
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© 1989 Kluwer Academic Publishers
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Lamers, H.J.G.L.M., Hoekzema, N., Trams, N.R., Cassatella, A., Barylak, M. (1989). AG Car: Variability, Extinction, Distance and Luminosity. 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_36
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DOI: https://doi.org/10.1007/978-94-009-1031-7_36
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