Abstract
Five planetary nebulae are known to show hydrogen-poor material nearthe central star. In the case of A58, this gas was ejected following alate thermal pulse similar to Sakurai's Object. In this paper I will reviewthese five objects. One of them, IRAS 18333 –2357, may not be a truePN. I will show that there is a strong case for a relation to the [WC]stars and their relatives, the weak emission-line stars. The surfaceabundances of the [WC] stars are explained via diffuse overshoot intothe helium layer. The hydrogen-poor PNe do not support this: theirabundances indicate a change of abundance with depth in the heliumlayer. A short-lived phase of very high mass loss, the r-AGB, isindicated. Sakurai's Object may be at the start of such a phase, and mayevolve to very low stellar temperatures.
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References
Alves, D.R., Bond, H.E. and Livio, M.: 2000, AJ 120, 2044.
Blöcker, T.: 2001, in: T. Blöcker, R. Waters and B. Zijlstra (eds.), Low Mass Wolf-Rayet Stars: Origin and Evolution, ApSS 275, 1.
Borkowski, K.J. and Harrington, J.P.: 1991, ApJ 379, 168.
Borkowski, K.J., Harrington, J.P. and Tsvetanov, Z.I.: 1995, ApJ 449, L143.
Borkowski, K.J., Tsvetanov, Z., Harrington, J.P. and Clegg, R.E.S.: 1993, ApJ 402, L57.
Dinerstein, H.L. and Lester, D.F.: 1984, ApJ 281, 702.
Dreizler, S. and Heber, U.: 1998, A&A 334, 618.
Gillet, F.C., Jacoby, G.H., Joyce, R.R., Cohen, J.G., Neugebauer, G., Soifer, B.T., Nakijima, T. and Matthews, K.: 1989, ApJ 338, 862.
Gillet, F.C., Neugebauer, G., Emerson, J.P. and Rice, W.L.: 1986, ApJ 300, 722.
Harrington, J.P.: 1996, in: C.S. Jeffery and U. Heber (eds.), Hydrogen-Deficient Stars, ASP Conference Series 96, p. 193.
Harrington, J.P., Borkowski, K.J. and Tsvetanov, Z.: 1995, ApJ 439, 264.
Harrington, J.P. and Paltoglou, G.: 1993, ApJ 411, L103.
Harris, W.E.: 1996, AJ 112, 1487.
Harris, W.E.: 1999, Catalog of Globular Clusters (http://physun.physics.mcmaster.ca/Globular.html)
Herwig, F., Blöcker, T., Langer, N. and Driebe, T.: 1999, A&A 349, L5.
Jacoby, G.H. and Ford, H.C.: 1983, ApJ 266, 298.
Kimeswenger, S., Kerber, F. and Weinberger, R.: MNRAS 296, 614.
Kingsburgh, R.L. and Barlow, M.J.: 1994, MNRAS 271, 257.
LeToeff, Y.: 2000, PhD thesis, UMIST
Manchado, A., Garcia-Lario, P. and Pottasch, S.R.: 1989, A&A 218, 267.
Manchado, A., Pottasch, S.R. and Mampaso, A.: 1988, A&A 191, 128.
Meaburn, J. and López, J.A.: 1996, ApJ 472, L45.
Meaburn, J., López, J.A., Bryce, M. and Redman, M.P.: 1998, A&A 334, 670.
Péquignot, D., Walsh, J.R., Zijlstra, A.A. and Dudziak, G.: 2000, A&A 361, L1.
Pollacco, D.L., Lawson, W.A., Clegg, R.E.S. and Hill, P.W.: 1992, MNRAS 257, 33P.
Pottasch, S.R., Mampaso, A., Manchado, A. and Menzies, J.W.: 1986, in: K. Hunger and D. Schönberner (eds.), Hydrogen-Deficient Stars and Related Objects, IAU Colloquium 87, p. 359.
Seitter, W.C.: 1987, ESO Messenger 50, 14.
Tylenda, R., Acker, A. and Stenholm, B.: 1993, A&AS 102, 595.
Zijlstra, A.A.: 2001, in: T. Blöcker, R. Waters and B. Zijlstra (eds.), Low Mass Wolf-Rayet Stars: Origin and Evolution, ApSS 275, 79.
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Zijlstra, A.A. Hydrogen-poor planetary nebulae. Astrophysics and Space Science 279, 171–182 (2002). https://doi.org/10.1023/A:1014633014448
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DOI: https://doi.org/10.1023/A:1014633014448