Abstract
In this work, two aspects of the chemical evolution of 4He in the Galaxy are considered on the basis of a sample of disk planetary nebulae (PN). First, an application of corrections owing to the contamination of 4He from the evolution of the progenitor stars shows that the He/H abundance by number of atoms is reduced by 0.012 to 0.015 in average, leading to an essentially flat He/H radial distribution. Second, a determination of the helium to heavy element enrichment ratio using the same corrections leads to values in the range 2.8 < ΔY / ΔZ < 3.6 for Y p = 0.23 and 2.0 < ΔY / ΔZ < 2.8 for Y p = 0.24, in good agreement with recent independent determinations and theoretical models.
Similar content being viewed by others
References
Allen, C., Carigi, L. and Peimbert, M.: 1998, Astrophys. J. 494, 247.
Amnuel, P.R.: 1993, Mon. Not. R. Astron. Soc. 261, 263.
Blöcker, T. and Schönberner, D.: 1990, Astron. Astrophys. 240, L11.
Boothroyd, A.I. and Sackmann, I.-J.: 1988, Astrophys. J. 328, 653.
Boothroyd, A.I. and Sackmann, I.-J.: 1999, Astrophys. J. 510, 232.
Burles, S., Nollett, K.M., Truran, J.N. and Turner, M.S.: 1999, Phys. Rev. Lett. 82, 4176.
Cazetta, J.O. and Maciel, W.J.: 2000, Rev. Mex. Astron. Astrofis. 36, 3.
Chiappini, C. and Maciel, W.J.: 1994, Astron. Astrophys. 288, 921.
Chiappini, C., Matteucci, F. and Gratton, R.: 1997, Astrophys. J. 477, 765.
Corradi, R.L.M., Perinotto, M., Schwarz, H.E. and Claeskens, J.F.: 1997, Astron. Astrophys. 322, 975.
Costa, R.D.D., Chiappini, C., Maciel,W.J. and Freitas-Pacheco, J.A.: 1996, Astron. Astrophys. Suppl. 116, 249.
Costa, R.D.D., Chiappini, C., Maciel, W.J. and Freitas-Pacheco, J.A.: 1997, in: R.T. Food and A. Renzini (eds.), Advances in stellar evolution, Cambridge, 159.
D'Odorico, S., Peimbert, M. and Sabbadin, F.: 1976, Astron. Astrophys. 47, 341.
Efremov, Y.N., Schilbach, E. and Zinnecker, H.: 1997, Astron. Nachr. 6, 335.
Esteban, C. and Peimbert, M.: 1995, Rev. Mex. Astron. Astrofis. SC 3, 133.
Esteban, C., Peimbert, M., Torres-Peimbert, S. and Garcia-Rojas, J.: 1999, Rev. Mex. Astron. Astrofis. 35, 65.
FaÚndez-Abans, M. and Maciel, W.J.: 1986, Astron. Astrophys. 158, 228.
Grevesse, N. and Sauval, A.J.: 1998, Space Sci. Rev. 85, 161.
Groenewegen, M.A.T. and de Jong, T.: 1993, Astron. Astrophys. 267, 410.
Groenewegen, M.A.T., van den Hoek, L.B. and de Jong, T.: 1995, Astron. Astrophys. 293, 381.
Gruenwald, R.B. and Viegas, S.M.M.: 1998, Astrophys. J. 501, 221.
Hajian, A.R., Balick, B., Terzian, Y. and Perinotto, M.: 1997, Astrophys. J. 487, 313.
Høg, E., Pagel, B.E.J., Portinari, L., Thejll, P.A., Macdonald, J. and Girardi, L.: 1998, Space Sci. Rev. 84, 115.
Izotov, Y.I., Thuan, T.X. and Lipovetsky, V.A.: 1997, Astrophys. J. Suppl. 108, 1.
Izotov, Y.I., Chaffee, F.H., Foltz, C.B., Green, R.F., Guseva, N.G. and Thuan, T.X.: 1999, Astrophys. J. 527, 757.
Kingsburgh, R.L. and Barlow, M.J.: 1994, Mon. Not. R. Astron. Soc. 271, 257.
Köppen, J., Acker, A. and Stenholm, B.: 1991, Astron. Astrophys. 248, 197.
Lequeux, J., Peimbert, M., Rayo, J.F., Serrano, A. and Torres-Peimbert, S.: 1979, Astron. Astrophys. 80, 155.
Liu, X.W. and Danziger, J.: 1993, Mon. Not. R. Astron. Soc. 263, 256.
Maciel, W.J.: 1988, Astron. Astrophys. 200, 178.
Maciel, W.J.: 1993, Astrophys. Space. Sci. 206, 285.
Maciel, W.J.: 1997, in: H.J. Habing and H.J.G.L.M. Lamers (eds.), IAU Symp. 180, Kluwer, 397.
Maciel, W.J.: 2000, in: F. Giovannelli and F. Matteucci (eds.), Chemical evolution of the Milky Way: stars versus clusters, Kluwer (in press).
Maciel, W.J. and Cazetta, J.O.: 1997, Astrophys. Space Sci. 249, 341.
Maciel, W.J. and Chiappini, C.: 1994, Astrophys. Space Sci. 219, 231.
Maciel, W.J. and Köppen, J.: 1994, Astron. Astrophys. 282, 436.
Maciel, W.J. and Quireza, C.: 1999, Astron. Astrophys. 345, 629.
Maciel, W.J. and Rocha-Pinto, H.J.: 1998, Mon. Not. R. Astron. Soc. 299, 889.
Maeder, A.: 1992, Astron. Astrophys. 264, 105.
Marigo, P.: 2000, in: F. Giovannelli and F. Matteucci (eds.), Chemical evolution of the Milky Way: stars versus clusters, Kluwer (in press).
Marigo, P., Bressan, A. and Chiosi, C.: 1996, Astron. Astrophys. 313, 545.
Matteucci, F. and Chiappini, C.: 1999, in: J.R.Walsh and M.R. Rosa (eds.), Chemical evolution from zero to high redshift, Springer, 83.
Matteucci, F. and François, P.: 1989, Mon. Not. R. Astron. Soc. 239, 885.
Méndez, R.H., Kudritzki, R.P. and Herrero, A.: 1992, Astron. Astrophys. 260, 329.
Méndez, R.H., Kudritzki, R.P., Herrero, A., Husfeld, D. and Groth, H.G.: 1988, Astron. Astrophys. 190, 113.
Olive, K.A., Steigman, G. and Walker, T.P.: 2000, Phys. Rep. (in press).
Padoan, P., Nordlund, Å. and Jones, B.J.T.: 1997, Mon. Not. R. Astron. Soc. 288, 145.
Pagel, B.E.J.: 1989, in: J.E. Beckman and B.E.J. Pagel (eds.), Evolutionary phenomena in galaxies, Cambridge, 368.
Pagel, B.E.J.: 1995, in: P. Crane (ed.), The light element abundances, Springer, 155.
Pagel, B.E.J. and Portinari, L.: 1998, Mon. Not. R. Astron. Soc. 298, 747.
Pagel, B.E.J., Simonson, E.A., Terlevich, R.J. and Edmunds, M.C.: 1992, Mon. Not. R. Astron. Soc. 255, 325.
Pasquali, A. and Perinotto, M.: 1993, Astron. Astrophys. 280, 581.
Peimbert, M.: 1978, in: Y. Terzian (ed.), IAU Symp. 76, Reidel, 215.
Peimbert, M.: 1979, in: W.B. Burton (ed.), IAU Symp. 84, Reidel, 307.
Peimbert, M.: 1990, Rep. Prog. Phys. 53, 1559.
Peimbert, M.: 1995, in: P. Crane (ed.), The light element abundances, Springer, 165.
Peimbert, M. and Serrano, A.: 1980, Rev. Mex. Astron. Astrofis. 5, 9.
Peimbert, M. and Torres-Peimbert, S.: 1974, Astrophys. J. 193, 327.
Peimbert, M. and Torres-Peimbert, S.: 1976, Astrophys. J. 203, 581.
Perinotto, M.: 1991, Astrophys. J. Suppl. 76, 687.
Perinotto, M., Purgathofer, A., Pasquali, A. and Patriarchi, P.: 1994, Astron. Astrophys. Suppl. 107, 495.
Renzini, A. and Voli, M.: 1981, Astron. Astrophys. 94, 175.
Rocha-Pinto, H.J., Scalo, J., Maciel, W.J. and Flynn, C.: 2000, Astrophys. J. Lett. 531, L115.
Sackmann, I.-J. and Boothroyd, A.I.: 1999, Astrophys. J. 510, 217.
Schönberner, D.: 1983, Astrophys. J. 272, 708.
Shaver, P.A., McGee, R.X., Newton, L.M., Danks, A.C. and Pottasch, S.R.: 1983, Mon. Not. R. Astron. Soc. 204, 53.
Stasińska, G., Gorny, S.K. and Tylenda, R.: 1997, Astron. Astrophys. 327, 736.
Stasińska, G. and Tylenda, R.: 1990, Astron. Astrophys. 240, 467.
Thuan, T.X. and Izotov, Y.I.: 1998, Space Sci. Rev. 84, 83.
van den Hoek, L.B. and Groenewegen, M.A.T.: 1997, Astron. Astrophys. Suppl. 123, 305.
Weidemann, V. and Koester, D.: 1983, Astron. Astrophys. 121, 77.
Zhang, C.Y.: 1993, Astrophys. J. 410, 239.
Author information
Authors and Affiliations
Rights and permissions
About this article
Cite this article
Maciel, W. Helium contamination from the progenitor stars of planetary nebulae: The He/H radial gradient and the ΔY / ΔZ enrichment ratio. Astrophysics and Space Science 277, 545–563 (2001). https://doi.org/10.1023/A:1013827617446
Issue Date:
DOI: https://doi.org/10.1023/A:1013827617446