Hostname: page-component-78c5997874-mlc7c Total loading time: 0 Render date: 2024-11-18T10:28:27.410Z Has data issue: false hasContentIssue false

AG Carinae and the WR Phenomenon in Luminous Blue Variables

Published online by Cambridge University Press:  03 August 2017

R. Viotti
Affiliation:
1Istituto Astrofisica Spaziale (CNR), Via E. Fermi 21, 00044 Frascati RM, Italy
G. B. Baratta
Affiliation:
2Osservatorio Astronomico, Viale del Parco Meilini 84, 00136 Roma
C. Rossi
Affiliation:
3Istituto Astronomico, Università La Sapienza, Via Lancisi 29, 00161 Roma
A. di Fazio
Affiliation:
3Istituto Astronomico, Università La Sapienza, Via Lancisi 29, 00161 Roma

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

AG Car is a Luminous Blue Variable which recently evolved from AIe to Ofpe/WN9 in four years at about constant bolometric luminosity, while in the visual the star faded by two magnitudes. This change is probably associated with variable opacity of an unstable massive expanding envelope of a hot star. We discuss the main spectral features of the star and of its ring nebula, and the spectral variations.

Type
Session VII. Evolution
Copyright
Copyright © Kluwer 1991 

References

Bandiera, R., Focardi, P., Altamore, A., Rossi, C., and Stahl, O. 1989, in: Physics of Luminous Blue Variables, Lamers, H. and de Loore, C. (eds.), Kluwer Academic Publishers, p. 279.CrossRefGoogle Scholar
Bensammar, S., Gaudenzi, S., Rossi, C., Johnson, H.M., Thé, P.S., Zuiderwijk, E.J., and Viotti, R. 1981, in: Effects of Mass Loss on Stellar Evolution, Chiosi, C. and Stalio, R. (eds.), Reidel, Dordrecht, p. 67.CrossRefGoogle Scholar
Caputo, F. and Viotti, R. 1970, Astron. Astrophys. 7, 266.Google Scholar
Friedjung, M. and Muratorio, G. 1987, Astron. Astrophys. 188, 100.Google Scholar
Hutsemekers, D. and Kohoutek, L. 1987, Astron. Astroph. Suppl. 73, 217.Google Scholar
Lamers, H.J.G.L.M. 1987, in: Instabilities in Luminous Early Type Stars, Lamers, H. and de Loore, C. (eds.), Reidel, Dordrecht, p. 99.CrossRefGoogle Scholar
Mayall, M.W. 1969, J. R. Astron. Soc. Canada 63, 221.Google Scholar
McGregor, P.J., Finlyason, K., and Hyland, A.R. 1988, Astrophys. J. 329, 874.CrossRefGoogle Scholar
Mila Mitra, P. and Dufour, R.J. 1990, Mon. Not. R. Astr. Soc. 242, 98.CrossRefGoogle Scholar
Paresce, F. and Nota, A. 1989, Astrophys. J. 341, L83.CrossRefGoogle Scholar
Sharov, A.S. 1975, in: Variable Stars and Stellar Evolution, Sherwood, W.A. and Plaut, J. (eds.), Reidel, Dordrecht, p. 275.CrossRefGoogle Scholar
Stahl, O. 1986, Astron. Astrophys. 164, 321.Google Scholar
Viotti, R. 1987, in: Instabilities in Luminous Early Stars, Lamers, H. and de Loore, C. (eds.), Reidel, Dordrecht, p. 257.CrossRefGoogle Scholar
Viotti, R., Altamore, A., Barylak, M., Cassatella, A., and Rossi, C. 1984, in: Future of Ultraviolet Astronomy Based on Six Years of IUE Research, NASA CP-2349, p. 23.Google Scholar
Viotti, R., Cassatella, A., Pontz, D., and Thé, P.S. 1988, Astron. Astrophys. 190, 333.Google Scholar
Viotti, R., Altamore, A., Rossi, C., and Cassatella, A. 1989, in: Physics of Luminous Blue Variables, Davidson, K. et al. (eds.), Kluwer Academic Publishers, Dordrecht, p. 268.CrossRefGoogle Scholar
Whitelock, P.A., Carter, B.S., Roberts, G., Whittet, D.G.B., and Baines, B.W.T. 1983, Mon. Not. R. Astr. Soc. 205, 577.CrossRefGoogle Scholar
Wolf, B. and Stahl, O. 1982, Astron. Astrophys. 112, 111.Google Scholar