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Carbon- and Oxygen-Rich Progenitors of Planetary Nebulae

Published online by Cambridge University Press:  07 August 2017

H.J. Habing  and
J.A.D.L. Blommaert
H.J. Habing
Affiliation:
Sterrewacht Leiden, P.O. Box 9513, 2300 RA Leiden, The Netherlands
J.A.D.L. Blommaert
Affiliation:
Sterrewacht Leiden, P.O. Box 9513, 2300 RA Leiden, The Netherlands

Extract

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This review concerns stars on the Asymptotic Giant Branch that are about to develop into planetary nebulae (=PNe). They are still termed “stars”, and properly so, and yet they have already, in statu nascendi, the structure of a PN. There are two different kinds: oxygen-rich stars (spectral class: M) and carbon-rich stars (spectral class: C).

Type
IV. Planetary Nebulae Connection: Evolution from the AGB
Information
Symposium - International Astronomical Union , Volume 155: Planetary Nebulae , 1993 , pp. 243 - 250
Copyright
Copyright © Kluwer 1993 

References

-Balick, B., Gonzalez, G., Frank, A., Jacoby, G. 1992, Astrophys. J. 392, 582.Google Scholar
-Bedijn, P.J. 1987, Astron. Astrophys. 186, 136.Google Scholar
-Bedijn, P.J. 1988, Astron. Astrophys. 205, 105.Google Scholar
-Benson, P.J., Little-Marenin, I., Woods, T.C., Attridge, J.M., Blais, K.A., Rudolph, D.B., Rubiera, M.E., Keefe, H.L. 1990, Astrophys. J. Suppl. Ser. 74, 911.Google Scholar
-Blanco, V.M. 1988, Astron. J. 95, 1400.Google Scholar
-Bowen, G.H., Willson, L.A. 1991, Astrophys. J. Lett. 375, L315.Google Scholar
-Chan, S.J., Kwok, S. 1988, Astrophys. J. 334, 362.Google Scholar
-Clegg, R.E.S., Peimbert, M., Torres-Peimbert, S. 1987, Month. Not. R.A.S. 224, 761.CrossRefGoogle Scholar
-Cutri, R.M., Low, F.J., Kleinmann, S.G., Olszewski, E.W., Willner, S.P., Campbell, B., Gillett, F.C. 1989, Astron. J. 97, 866.Google Scholar
-Egan, M.P., Leung, C.M. 1991, Astrophys. J. 383, 314.CrossRefGoogle Scholar
-Elitzur, M. 1992, Astronomical Masers (Kluwer Publ., Dordrecht).CrossRefGoogle Scholar
-Frogel, J.A., Mould, J., Blanco, V.M. 1990, Astrophys. J. 352, 96.Google Scholar
-Griffin, I.P. 1990, Mon. Not. R.A.S. 247, 591.Google Scholar
-Groenewegen, M.A.T., de Jong, T., van der Bliek, N.S., Slijkhuis, S., Willems, F.J.: 1992 Astron. Astrophys. 253, 150.Google Scholar
-Hughes, S.M.G. 1989, Astron. J. 97, 1634.Google Scholar
-Hughes, S.M.G., Wood, P.R., 1990, Astron. J. 99, 784.Google Scholar
-Iben, I. ApJ Suppl. Ser. 1991 76, 55.Google Scholar
-Justtanont, K., Tielens, A.G.G.M. 1992, Astrophys. J. 389, 400.Google Scholar
-Kastner, J.H. 1992 Astrophys. J. (december 10 issue) Google Scholar
-Loup, C., Forveille, T., Omont, A., Paul, J.F. Astron. Astrophys. Suppl. Ser. 1992 (in press) Google Scholar
-Mennessier, M.O., Omont, A. 1990 (editors) From Mira's to Planetary Nebulae: Which path for stellar evolution? Editions Frontiéres (Gif sur Yvette).Google Scholar
-Olofsson, H., Carlström, U., Eriksson, K., Gustafsson, B., Willson, L. 1990, Astron. Astrophys. Lett. 230, L13.Google Scholar
-Omont, A., Loup, C., Forveille, T., te Lintel-Hekkert, P., Habing, H., Sivagnanam, P. 1992 Astron. Astrophys. (in press) Google Scholar
-Plaut, L. 1970, Astron. Astrophys. 8, 341.Google Scholar
-Reid, N. 1991, Astrophys. J. 382, 143.Google Scholar
-Reid, N., Tinney, C., Mould, J. 1990, Astrophys. J. 348, 98.CrossRefGoogle Scholar
-Reid, N., Glass, I., Catchpole, R.M., 1988, Mon. Not. R.A.S. 232, 53.Google Scholar
-Reid, N., Mould, J. 1984, Astrophys. J. 284, 98.CrossRefGoogle Scholar
-Reid, N., Mould, J. 1990, Astrophys. J. 360, 490.Google Scholar
-Renzini, A., Voli, M. 1981, Astron. Astrophys. 94, 175.Google Scholar
-Rowan-Robinson, M., Harris, S. 1983, Mon. Not. R.A.S. 202, 767.Google Scholar
-Sahai, R. 1990, Astrophys. J. 362, 652.Google Scholar
-Shklovskii, I.S. 1956, Astron. Zh. 53, 315.Google Scholar
-Terndrup, D.M., Frogel, J.A., Whitford, A.E.: 1991, Astrophys. J. 378, 742 CrossRefGoogle Scholar
-van der Veen, W.E.C.J., Habing, H.J. 1988, Astron. Astrophys. 194, 125.Google Scholar
-van der Veen, W.E.C.J., Habing, H.J. 1990, Astron. Astrophys. 231, 404.Google Scholar
-Weidemann, V. 1990, Ann. Rev. Astron. Astrophys. 28, 103.Google Scholar
-Wesselink, T. 1987, thesis Katholieke Universiteit van Nijmegen (the Netherlands).Google Scholar
-Westerlund, B.E., Lequeux, J., Azzopardi, M., Rebeirot, E., 1991, Astron. Astrophys. 244, 367.Google Scholar
-Whitelock, P., Feast, M., Catchpole, R. 1991, Mon. Not. R.A.S. 248, 276.CrossRefGoogle Scholar
-Willems, F.J., de Jong, T. 1986, Astron. Astrophys. 196, 173.Google Scholar
-Wood, P.R., Vassiliadis, E. 1992, in Highlights of Astronomy 9, tbd. Google Scholar
-Wood, P., Whiteoak, J., Hughes, S., Bessell, M., Gardner, F., Hyland, A. (preprint) Google Scholar
-Zijlstra, A.A., Loup, C., Waters, L.B.F.M., de Jong, T. 1992 Astron. Astrophys. Lett. (submitted) Google Scholar