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Wind Features and Wind Velocities

Published online by Cambridge University Press:  19 July 2016

Michael Grewing
Michael Grewing*
Affiliation:
Astronomisches Institut der Universität, Waldhäuserstrasse 64, D-7400 Tübingen, Germany, Fed. Rep.

Abstract

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Fast winds have been detected in the spectra of many nuclei of planetary nebulae (PNNi). The wind velocities range from about 600 km/s to roughly 4000 km/s. While these winds add little to the mass of the nebular shells they may significantly effect their internal kinematics.

By studying the emission from the faint outer envelopes of PNe one can infer also the wind properties of the progenitors of the current nuclei. This will in the end allow to test quantitatively current models of the origin of PNe.

Type
III. Central Stars
Information
Symposium - International Astronomical Union , Volume 131: Planetary Nebulae , 1989 , pp. 241 - 250
Copyright
Copyright © Kluwer 1989 

References

Adam, J., and Köppen, J.: 1985, Astron.Astrophys. 142, 461 Google Scholar
Abbott, D.C.: 1982, Astrophys.J. 259, 282 CrossRefGoogle Scholar
Bässgen, M., Bässgen, G., Barnstedt, J., Grewing, M., Bianchi, L. Mitt. Astron.Ges. 67, 342 Google Scholar
Bianchi, L., Cerrato, S., and Grewing, M.: 1986, Astron. Astrophys. 169, 227 Google Scholar
Bianchi, L., and Grewing, M.: 1987, Astron.Astrophys. 181, 85 Google Scholar
Bombeck, G., Köppen, J., and Bastian, U.: 1986, in ‘New Insights in Astrophysics’, ESA SP-263, p.287 Google Scholar
Cerruti-Sola, M., and Perinotto, M.: 1985, Astrophys.J. 291, 237 CrossRefGoogle Scholar
Chu, Y.-H., Jacoby, G.H., and Arendt, R.: 1987, Astrophys.J.Suppl.Ser. 64, 529 Google Scholar
Ferch, R.L., and Salpeter, E.E.: 1975, Astrophys.J. 202, 195 Google Scholar
Gieseking, F., Becker, I., and Solf, J.: 1986, Astrophys.J. 295, L17 Google Scholar
Gieseking, F., and Solf, J.: 1986, Astron.Astrophys. 163, 174 Google Scholar
Heap, S.R., Bogess, A., Holm, A., Klinglesmith, D.A., Sparks, W., West, D., Wu, C.C., Boksenberg, A., Willis, A., Wilson, R., Macchetto, F., Selvelli, P.L., Stickland, D., Greenstein, J.L., Hutchings, J.B., Underhill, A.B., Viotti, R., and Whelan, J.A.J.: 1978, Nature 275, 385 Google Scholar
Heap, S.: 1983, IAU Symp. 103, p. 375 Google Scholar
Heap, S.: 1986, in ‘New Insights in Astrophysics’, ESA SP-263, p. 291 Google Scholar
Hippelein, H.H., Bässgen, M., and Grewing, M.: 1985, Astron.Astrophys. 152, 213 Google Scholar
Kaler, J.B., Feibelman, W.A., and Henrichs, H.F.: 1987, IAP 87-15 (Preprint) Google Scholar
Kwok, S., Fitzgerald, P.M., and Purton, C.R.: 1978, Astrophys.J. 219, L125 Google Scholar
Mathews, W.G.: 1966, Astrophys.J. 143, 173 CrossRefGoogle Scholar
Mendez, R.H., Kudritzki, R.P., Gruschinkske, J., Simon, K.P.: 1981, Astron. Astrophys. 101, 323 Google Scholar
Mendez, R.H., Kudritzki, R.P., Herrero, A., Husfeld, D., Groth, H.G.: 1987, Astron. Astrophys. (in press) Google Scholar
O'Dell, C.R., and Ball, M.E.: 1985, Astrophys.J. 289, 526 Google Scholar
Perinotto, M.: 1983, IAU Symp. 103, 343 Google Scholar
Phillips, J.P., Mampaso, A., Riera, A.: 1987, IAU Symp. 131, B32 Google Scholar
Sofia, S., and Hunter, J.H.: 1968, Astrophys.J. 152, 405 Google Scholar
Taylor, A.R., Pottasch, S.R., and Zhang, C.Y.: 1987, Astron.Astrophys. 171, 178 Google Scholar
Weinberger, R.: 1987, Preprint Google Scholar