Hostname: page-component-cd9895bd7-mkpzs Total loading time: 0 Render date: 2024-12-19T02:52:33.947Z Has data issue: false hasContentIssue false
  • English
  • Français

Is Superficial Knowledge about Stellar Surfaces Sufficient?

Published online by Cambridge University Press:  12 April 2016

Bengt Gustafsson
Bengt Gustafsson*
Affiliation:
Astronomiska Observatoriet, Box 515, S-751 20 Uppsala, Sweden

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.

The significance of a detailed knowledge of the atmosphere of a star for a proper understanding of its interior is illustrated and discussed. It is concluded that significant progress in the understanding of stellar atmospheres is needed in order to match methods, discoveries and needs in the study of stellar internal structure and evolution.

Type
II. Atmospheres, a window to the interior
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 122 - 135
Copyright
Copyright © Astronomical Society of the Pacific 1993

References

Balmforth, N.J. 1992a, b, c, M.N.R.A.S. 255, 603, 632, 639.Google Scholar
Bell, R.A., Eriksson, K., Gustafsson, B., Nordlund, Å. 1976, A.&Ap. Suppl. 23, 37.Google Scholar
Cannon, C.J., Thomas, R.N. 1977, Ap.J. 211, 910.CrossRefGoogle Scholar
Cattaneo, F., Brummell, N.H., Toomre, J., Malagou, A., Hurlburt, N.E. 1991, Ap.J. 370, 282.CrossRefGoogle Scholar
Charbonneau, R., MacGregor, K.B. 1992a, Ap.J. 387, 639.Google Scholar
Charbonneau, R., MacGregor, K.B. 1992b, Ap.J. Letters, submitted.Google Scholar
Christensen-Dalsgaard, J., Gough, D.O. 1982, M.N.R.A.S. 198, 141.Google Scholar
Christensen-Dalsgaard, J., Frandsen, S. 1983, Solar. Phys. 82, 165.Google Scholar
Cram, L.E. 1989, in Cram and Kuhi 1989, p. 181.Google Scholar
Cram, L.E., Kuhi, L.V. 1989 (eds.), FKG stars and T Tauri Stars, Monograph Series on Nonthermal Phenomena in Stellar Atmospheres, NASA SP-502.Google Scholar
Edvardsson, B., Andersen, J., Gustalsson, B., Lambert, D.L., Nissen, P.E., Tomkin, J. 1992, A.&Ap., to be submitted.Google Scholar
Eriksson, K., Gustafsson, B., Jørgensen, U.G., Nordlund, Å. 1986, A.&Ap. 132, 37.Google Scholar
Gehren, T. 1988, in Rev. Mod. Astron. 1, 52, Klare, G. (ed.) (Springer: Heidelberg).Google Scholar
Gough, D.O., Weiss, N.O. 1976, M.N.R.A.S. 176, 589.Google Scholar
Gough, D., Toomre, J. 1991, Arm. Rev. A. Ap. 29, 627.Google Scholar
Gustafsson, B., Bell, R.A., Eriksson, K., Nordlund, Å. 1975, A.&Ap. 42, 407.Google Scholar
Gustafsson, B., Jørgensen, U.G. 1985, in Proc. lAU Symp. 111: Calibration of Fundamental Stellar Quantities, Hayes, D.S., Pasinetti, L.E., Philip, A.G.D. (eds.) (Reidel: Dordrecht) p. 303.Google Scholar
Holweger, H. 1970, A.&Ap. 4, 11.Google Scholar
Jørgensen, U.G. 1992, Rev. Mex. A. Ap., in press.Google Scholar
Kawaler, S.D. 1988, Ap.J. 333, 236.Google Scholar
Kurucz, R. 1991, in Stellar Atmospheres: Beyond Classical Models, Crivellari, L., Hubeny, I., Hummer, D.G. (eds.), NATO ASI-Series C 341.Google Scholar
Lambert, D.L. 1989, in Cosmic Abundances of Matter, Jake Waddington, C. (ed.), AIP Conf. Proc. 183, 168.Google Scholar
Libbrecht, K.G., Popp, B.D., Kaufman, J.M., Penn, M.J. 1986, Nature 323, 235.Google Scholar
Mestel, L. 1984, in 3rd Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, Baliunas, S.L., Hartmann, L. (eds.) (Springer: New York), p. 49.CrossRefGoogle Scholar
Mestel, L., Weiss, N.O. 1987, M.N.R.A.S. 226, 123.Google Scholar
Michaud, G. 1991, in Proc. IAU Symp. 145, Evolution of Stars: The Photospheric Abundance Connection, Michaud, G., Tutukov, A. (eds.) (Kluwer Acad.: Dordrecht), p. 111.Google Scholar
Nordlund, Å., Dravins, D. 1990, A.&Ap. 228, 155.Google Scholar
Nordlund, Å., Stein, R.F. 1991a, in Stellar Atmospheres: Beyond Classical Models, Crivellari, L., Hubeny, I., Hummer, D.G. (eds.), NATO ASI-Series C 341, 263.Google Scholar
Nordlund, Å., Stein, R.F. 1991b, Proc. of the Mini Workshop on the Solar 5 Minutes Oscillations, Univ. of Oslo.Google Scholar
Nordlund, Å., Brandenburg, A., Jennings, R.J., Rieutord, M., Ruokolainen, J., Stein, R.F., Tuominen, I. 1992, Ap.J. 392, 647.Google Scholar
Pedersen, B.B., VandenBerg, D.A., Irwin, A.W. 1990, Ap.J. 352, 279.Google Scholar
Pinsonneault, M.H., Kawaler, S.D., Sofia, S., Demarque, P. 1989, Ap.J. 338, 424.CrossRefGoogle Scholar
Sackmann, I.-J., Boothroyd, A.I. 1991, Ap.J. 366, 529.Google Scholar
Schatzman, E. 1962, Ann. d’Astrophys. 25, 18.Google Scholar
Schwarzschild, M. 1958, Structure and Evolution of the Stars,(Princeton Univ. Press).Google Scholar
Spite, M., Spite, F. 1985, Ann. Rev. A. Ap. 23, 225.Google Scholar
Stein, R.F., Nordlund, Å. 1989, Ap.J. Letters 342, L95.Google Scholar
Stein, R.F., Nordlund, Å. 1991, in Challenges to Theories of the Structure of Moderate Mass Stars, Toomre, J. and Gough, D.O. (eds.), Lecture Notes in Physics 388, 195 (Springer: Heidelberg).Google Scholar
Thomas, R.N. 1989, in Cram and Kuhi (1989), p. ix.Google Scholar
Vainshtein, S.I., Zeldovich, Ya.B., 1972, Sov. Phys. Usp. 15, 159.Google Scholar
VandenBerg, D.A. 1983, Ap.J. Suppl. 51, 29.Google Scholar
VandenBerg, D.A. 1992, private communication.Google Scholar
VandenBerg, D.A., Laskarides, P.G. 1987, Ap.J. Suppl. 64, 103.Google Scholar
Wheeler, J.C., Sneden, C., Truran, J.W. Jr., 1989, Ann. Rev. A. Ap. 27, 279.Google Scholar
Zahn, J.-P. 1992, A.&Ap., submitted.Google Scholar