Hostname: page-component-cd9895bd7-dzt6s Total loading time: 0 Render date: 2024-12-23T19:04:24.705Z Has data issue: false hasContentIssue false

36. Theory of Stellar Atmospheres (Theorie Des Atmospheres Stellaires)

Published online by Cambridge University Press:  25 April 2016

Abstract

Image of the first page of this content. For PDF version, please use the ‘Save PDF’ preceeding this image.'
Type
Meeting Report
Copyright
Copyright © Kluwer 1994

References

CH91: Mechanisms of Chromospheric and Coronal Heating, Ulmschneider, P., Priest, E.R., and Rosner, R. (Eds.), 1991, Springer-Verlag: Berlin.CrossRefGoogle Scholar
MD91: The Sun and Cool Stars: Activity, Magnetism, Dynamos, Tuominen, I., Moss, D., Rüdiger, G. (Eds.): 1991, Springer-Verlag: Berlin.CrossRefGoogle Scholar
AM91: Angular Momentum Evolution of Young Stars, Catalano, S., and Stauffer, J.R. (Eds.), 1991, Kluwer: Dordrecht.CrossRefGoogle Scholar
SI92: Surface Inhomogeneities on Late-Type Stars, Byrne, P.B., and Mullan, D.J. (Eds.), 1992, Springer-Verlag: Berlin.CrossRefGoogle Scholar
SC92: Solar and Stellar Coronae, Pallavicini, R. (Ed.), 1992, Memorie Soc. Astron. Ital. 64, No. 3-4.Google Scholar
CS92: Seventh Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Giampapa, M.S., and Bookbinder, J.A. (Eds.), 1992, Astron. Soc. Pacific: San Francisco.Google Scholar
SC93: Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium, Linsky, J.A., and Serio, S. (Eds.), 1993, Kluwer: Dordrecht.CrossRefGoogle Scholar
Baliunas, S.: 1991, in The Sun in Time (Sonett, C.P., Giampapa, M.S., and Matthews, M.S. eds.), University of Arizona: Tucson, p. 809.Google Scholar
Feigelson, E.D., Giampapa, M.S., and Vrba, F.J.: 1991, in The Sun in Time (Sonett, C.P., Giampapa, M.S., and Matthews, M.S. eds.), University of Arizona: Tucson, p. 658.Google Scholar
Haisch, B.M., Strong, K.T., and Rodonò, M.: 1991, Ann. Rev. Astron. Ap. 29, 275.CrossRefGoogle Scholar
Kuijpers, J.: 1993, in The Sun: A Laboratory for Astrophysics (Schmeltz, J.T. and Brown, J.G. eds.), Kluwer:Dordrecht, p. 535.Google Scholar
Landstreet, J.D.: 1992, Ann. Rev. Astron. Ap. 4, 35.Google Scholar
Pallavicini, R.: 1992a,b, in The Sun: A Laboratory for Astrophysics (Schmeltz, J.T. and Brown, J.C. eds.), Kluwer: Dordrecht, pp. 313 and 509.CrossRefGoogle Scholar
Pettersen, B.R. (Ed.): 1991, Stellar Flares, special issue of Memorie Soc. Astron. Ital, Vol. 62, No. 2.Google Scholar
Radick, R.R.: 1991, in The Sun in Time (Sonett, C.P., Giampapa, M.S., and Matthews, M.S. eds.), University of Arizona: Tucson, p. 787.Google Scholar
Schrijver, C.J.: 1993, in Inside the Stars, proceedings of IAU Colloquium No. 137, Vienna: April 1992.CrossRefGoogle Scholar
Strassmeier, K.G., Hall, D.S., Fekel, F.C., and Scheck, M.: 1993, Astron. Astrophys. Suppl. 100, 173.Google Scholar
Baliunas, S.L. & Jastrow, R. 1993. Energy: The International Journal, in print.Google Scholar
Byrne, P., & Mullan, D. (eds.) 1991. Surface Inhomogeneities in Late-Type Stars, (Springer: Berlin)Google Scholar
Cattaneo, F. & Malagoli, A. 1992. Seventh Cambridge Worshop on Cool Stars, Stellar Systems, and the Sun, (Ast. Soc. Pacific: San Francisco), Giampapa, M.S. & Bookbinder, J.A., eds., p. 139.Google Scholar
Cochran, W.D. & Hatzes, A.P. 1993. Ap. Space Sci. in print.Google Scholar
Donahue, R.A. & Baliunas, S.L. 1992. Ap.J. 393, L63.CrossRefGoogle Scholar
Eaton, J.A., Henry, G.W., Bell, C., & Okorogu, A. 1993. Astron. J., submitted.Google Scholar
Foukal, P. & Lean, J. 1990. Science 247, 504.CrossRefGoogle Scholar
Fröhlich, C., Foukal, P.V. Hickey, J.R. Hudson, H.S., & Wilson, R.C. 1991. The Sun in Time, (Univ. Arizona: Tucson), Sonett, C.P., Giampapa, M.S., Mathews, M.S., eds., p. 11.Google Scholar
Gray, D.F. 1988. Lectures on Spectral-Line Analysis: F, G, and K Stars, (The Publisher: Arva, Ontario).Google Scholar
Gray, D.F. 1994. Publ. Astron. Soc. Pacific, submitted.Google Scholar
Gray, D.F., Baliunas, S.L., Lockwood, G.W., & Skiff, B.A. 1993. Ap.J. 400, 681.CrossRefGoogle Scholar
Gray, D.F. & Nagel, T. 1988. Ap.J., 341, 421426.CrossRefGoogle Scholar
Hossain, M. & Mullan, D.J. 1991. Ap.J. 380, 631.CrossRefGoogle Scholar
Jankov, S. & Foing, B.H. 1992. Astron. Ap. 256, 533.Google Scholar
Kim, Y.-C. & Fox, P.A. 1992. Seventh Cambridge Worshop on Cool Stars, Stellar Systems, and the Sun (Ast. Soc. Pacific: San Francisco), Giampapa, M.S. & Bookbinder, J.A. eds., 172.Google Scholar
Kuhn, J.R. 1991. Adv. Space Res. 11, (4)171.CrossRefGoogle Scholar
Larson, A.M., Irwin, A.W., Yang, S.L.S., Goodenough, C., Walker, G.A.H., Walker, A.R., & Bohlender, D.A. 1993. Publ. Astron. Soc. Pacific, submitted.Google Scholar
Livingston, W. & Steffen, M. 1988. Adv. Space Res. 8, 133.Google Scholar
Lou, Y.Q. 1992. Ap.J. 395, 682.CrossRefGoogle Scholar
Pap, J.M. (ed.) 1994. The Sun as a Variable Star: Solar and Stellar Irradiance Variations, (Cambridge: Cambridge).CrossRefGoogle Scholar
Radick, R.R., Lockwood, G.W., & Baliunas, S.L. 1990. Science 247, 39.CrossRefGoogle Scholar
Ribes, E., Beardsley, B., Brown, T.M., DeLanche, Ph., Laclare, F., Kuhn, J.R., & Leister, N.V. 1991. The Sun in Time, (Univ. Arizona: Tucson), Sonett, C.P., Giampapa, M.S., Mathews, M.S., eds., 59.Google Scholar
Rosner, R., An, C.-H., Musielak, Z.E., Moore, R.L., & Suess, S.T. 1991. Ap.J. Lett. 372, L91.Google Scholar
Smith, P.H., McMillan, R.S., & Merline, W.J. 1987. Ap.J. 317, L79.CrossRefGoogle Scholar
Sofia, S. 1994. in The Sun as a Variable Star: Solar and Stellar Irradiance Variations, (Cambridge: Cambridge).Google Scholar
Spruit, H.C., Nordlund, , & Title, A.M. 1990. Ann. Rev. Ast. Ap. 28, 263.CrossRefGoogle Scholar
Stein, R.F., Brandenburg, A., & Nordlund, 1992. Seventh Cambridge Worshop on Cool Stars, Stellar Systems, and the Sun, (Ast. Soc. Pacific: San Francisco), Giampapa, M.S. & Bookbinder, J.A., eds., 148.Google Scholar
Ulmschneider, P., Záhringer, K., & Musielak, Z.E. 1991, Astron. Ap. 106, 9.Google Scholar
[1] Ayres, T.R., et al. 1994, submitted to ApJ.Google Scholar
[2] Benz, A.O. and Alef, W. 1991, Astr. Ap. 252, L19.Google Scholar
[3] Bookbinder, J.A. 1991, Mem S.A.It 62, 321.Google Scholar
[4] Brown, A., et al. 1991, Ap. J. 373, 614.Google Scholar
[5] Chiuderi-Drago, F. and Franciosini, E. 1993, ApJ, in press.Google Scholar
[6] Dempsey, R.C., Linsky, J.L., Fleming, T.A., and Schmitt, J.H.M.M., 1993a, Ap. J. S. 86, 599.CrossRefGoogle Scholar
[7] Dempsey, R.C., Linsky, J.L., Schmitt, J.H.M.M., and Fleming, T.A., 1993b, Ap. J. 413, f333.CrossRefGoogle Scholar
[8] Drake, S.A., Simon, T., and Linsky, J.L. 1992, Ap. J. S. 82, 311.CrossRefGoogle Scholar
[9] Drake, S.A., et al. 1993, ApJ, in press.Google Scholar
[10] Doyle, J.G., et al. 1991, M.N.R.A.S. 248, 503.CrossRefGoogle Scholar
[11] Elias, N.M. and Güdel, M. 1993, A. J. 106, 337.CrossRefGoogle Scholar
[12] Elvis, M. 1990, Imaging X-ray Astronomy: A Decade of Einstein Observatory Achievements (Cambridge: Cambridge U. Press).Google Scholar
[13] Feldman, U. 1992, Physica Scripta 46, 202.CrossRefGoogle Scholar
[14] Feldman, U., et al. 1992, Ap. J. S. 81, 387.CrossRefGoogle Scholar
[15] Fleming, T.A., et al. 1993, Ap. J. 410, 387.CrossRefGoogle Scholar
[16] Fox, D., et al. 1994, A&A, in press.Google Scholar
[17] Gorenstein, P and Zombeck, M. 1990, High Resolution X-ray Spectroscopy of Cosmic Plasmas (Cambridge: Cambridge U. Press).Google Scholar
[18] Grillo, F., et al. 1992, Ap. J. S. 81, 795.CrossRefGoogle Scholar
[19] Güdel, M. 1994, ApJS, in press.Google Scholar
[20] Güdel, M. and Benz, A.O. 1993, Ap. J. (Letters) 405, L63.CrossRefGoogle Scholar
[21] Güdel, M., et al. 1993, ApJ, in press.Google Scholar
[22] Haisch, B., et al. 1991, Ap. J. (Letters) 383, L15.CrossRefGoogle Scholar
[23] Linsky, J.L. 1991, Mem S.A.It 62, 307.Google Scholar
[24] Linsky, J.L., Drake, S.A., and Bastian, T.S. 1992, Ap. J. 393, 341.CrossRefGoogle Scholar
[25] Linsky, J.L. and Serio, S. 1993, Physics of Solar and Stellar Coronae: G.S. Vaiana Memorial Symposium (Dordrecht: Kluwer).CrossRefGoogle Scholar
[26] Maggio, A., et al. 1990, Ap. J. 348, 253.CrossRefGoogle Scholar
[27] Malina, R.F. and Bowyer, S. 1991, in Extreme Ultraviolet Astronomy, ed. Malina, R.F. and Bowyer, S. (New York: Pergamon), 397.Google Scholar
[28] Malina, R. et al. 1993, ApJ, in press.Google Scholar
[29] Maran, S.P., et al. 1994, ApJ, in press.Google Scholar
[30] Massi, M. and Chiuderi-Drago, F. 1991, Astr. Ap. 253, 403.Google Scholar
[31] Micela, G., et al. 1990, Ap. J. 348, 557.CrossRefGoogle Scholar
[32] Morris, D.H., Mutel, R,L., and Su, B. 1990, Ap. J. 362, 299.CrossRefGoogle Scholar
[33] Pallavicini, R. 1989, A&A Reviews 1, 177.Google Scholar
[34] Pallavicini, R. 1991, in The Sun: a Laboratory for Astrophysics, ed. Brown, J.C. and Schmelz, J.T..Google Scholar
[35] Pallavicini, R., Tagliaferri, G., and Stella, L. 1990, Astr. Ap. 228, 403.Google Scholar
[36] Patten, B.M. and Simon, T. 1993, to appear in ApJL.Google Scholar
[37] Pfeffermann, E., et al. 1987, in Soft X-ray Optics and Technology, Proc. SPIE 733, 519.CrossRefGoogle Scholar
[38] Pounds, , et al. 1993, M.N.R.A.S. 260, 77.CrossRefGoogle Scholar
[39] Reimers, D. and Schmitt, J.H.M.M 1992, Ap. J. (Letters) 392, L55.CrossRefGoogle Scholar
[40] Schmitt, J.H.M.M., et al. 1990a, Ap. J. 365, 704.CrossRefGoogle Scholar
[41] Schmitt, J.H.M.M., et al. 1990b, Ap. J. 351, 492.CrossRefGoogle Scholar
[42] Schmitt, J.H.M.M., et al. 1993, Ap. J. (Letters) 402, L13.CrossRefGoogle Scholar
[43] Siarkowski, M. 1992, MNRAS 259, 453.CrossRefGoogle Scholar
[44] Simon, T. and Drake, S.A. 1993, to appear in AJ.Google Scholar
[45] Stern, R.A., et al. 1992, Ap. J. (Letters) 399, L159.CrossRefGoogle Scholar
[46] Trümper, J., et al. 1983, Nature 349, 579.CrossRefGoogle Scholar
[47] Ulmschneider, P., Priest, E.R., and Rosner, R. 1990, Mechanisms of Chromospheric and Coronal Heating (Berlin: Springer-Verlag).Google Scholar
[48] Umana, G., Catalano, S., and Rodono, M. 1991, Astr. Ap. 249, 217.Google Scholar
[49] Usov, V.V. and Melrose, D.B. 1992, Ap. J. 395, 575.CrossRefGoogle Scholar
[50] Wood, B.E., Brown, A., and Linsky, J.L. 1993a, submitted to ApJ.Google Scholar
[51] Wood, B.E., et al. 1993b, submitted to ApJS.Google Scholar
Bjorkman, J. E. and Cassinelli, J. P. (1993). Formation Around Rotating Stars Due to Ram Pressure Confinement by the Stellar Wind. Ap. J. 409, 429449.CrossRefGoogle Scholar
Bowen, G. H. and Willson, L. A. (1991). From Wind to Superwind: The Evolution of Mass-Loss Rates for Mira Models. Ap. J. 375, 153L56.CrossRefGoogle Scholar
Boyd, C. J. and Marlborough, J. M. (1991). Continuum Polarization by Electron Scattering in Rotationally Distorted, Radiation-Driven Stellar Winds: B[e] Supergiants. Ap. J. 369: 191199.CrossRefGoogle Scholar
Chen, H., Marlborough, J. M., and Waters, L. B. F. M. (1992). Dynamics of the Envelopes of Be Stars in the Equatorial Plane. Ap. J. 384, 605612.CrossRefGoogle Scholar
Dravins, D. (1990). Stellar granulation VI. Four-component models and non-solar-type stars. Astr. Ap. 228, 218230.Google Scholar
Drew, J. E. (1990). Relation Between Mass-Loss Rate and H-alpha Emission for O Star Winds. Ap. J. 357, (No 2), 573581.CrossRefGoogle Scholar
Fleischer, A. J., Gauger, A., and Sedlmayr, . (1992). Circumstellar dust shells around long-period variables. I. Dynamical Models of C-stars Including Dust Formation, Growth and Evaporation. Astr. Ap. 266, 321339.Google Scholar
Fokin, A. B. (1992). Shock waves and H-alpha profiles in the hydrodynamical model of RR Lyrae‘. M. N. R. S. 256, 2636.Google Scholar
Gail, H.-P., Cuntz, M., and Ulmschneider, . (1990). Wave pressure in stellar atmospheres due to shock wave trains. Astr. Ap. 234, 359365.Google Scholar
Goeres, A. and Sedlmayr, E. (1992). “The envelopes of R Coronae Borealis stars I. A physical model of the decline events due to dust formation”, A & A 265, 216236.Google Scholar
Hofner, S. and Dorfi, E. A. (1992). Dust formation in winds of long-period vaariables II. dust energetics, optical properties, chemistry, time scales. Astr. Ap. 265 (No 1), 207215.Google Scholar
Hummer, D. G. and Rybicki, G. B. (1992). The Sobolev approximation for line formation with partial frequency redistribution. Ap. J. 387, 248257.CrossRefGoogle Scholar
Koninx, J.-P. M. and Pijpers, F. P. (1992). The applicability of the linearized theory of sound-wave driven winds. Astr. Ap. 265, 183195.Google Scholar
Kudritzki, R. P. (1992). The formation of weak metal lines in the atmospheres of O-stars. The role of microturbulence and transonic matter outflow. Astr. Ap. 266, 395401.Google Scholar
Lobel, A., Achmad, L., Jager, de and Nieuwenhuizen, . (1992). On the instability parameters of stellar atmosphers. Astr. Ap. 264, 147152.Google Scholar
Lucy, L. B. and Abbott, D. C. (1993). Multiline transfer and the dynamics of Wolf-Rayet winds. Ap. J. 405, 738746 CrossRefGoogle Scholar
Mazzali, P. A. (1990). The effect of stellar rotation on the properties of a radiatively driven stellar wind. Astr. Ap. 238, 191206.Google Scholar
Netzer, N. and Elitzur, M. (1992). The dynamics of stellar outflows dominated by interaction of dust and radiation. Ap. J. 410, 701713.CrossRefGoogle Scholar
Nordlund, Å. and Dravins, D. (1990). Stellar granulation III. Hydrodynamic model atmospheres. Astr. Ap. 228, 155183.Google Scholar
Owocki, S. P. and Rybicki, G. B. (1990). Instabilities in line-driven stellar winds. V. Effect of an optically thick continuum. Ap. J. 368, 261263.CrossRefGoogle Scholar
Owocki, S. P. and Zank, G. P. (1991). The effect of viscosity on steady transonic flow with a nodal solution topology. Ap. J. 368, 491503.CrossRefGoogle Scholar
Poe, C. H., Owocki, S. P., and Castor, . (1990). The steady state solutions of radiatively driven stellar winds for a non-Sobolev, pure absorption model. Ap. J. 358, 199213.CrossRefGoogle Scholar
Taylor, M. and Cassinelli, J. P. (1992). Polarization cancellation in the two-component winds from Wolf-Rayet stars. Ap. J. 401, 311316.CrossRefGoogle Scholar
Velli, M. (1993). On the propagation of ideal, linear Alfvén waves in radially stratified stellar atmospheres and winds. A & A 270: 304314.Google Scholar
[1] Adams, F. C., Ruden, S. P., & Shu, F. H. 1989, ApJ, 347, 959 CrossRefGoogle Scholar
[2] Adams, F. C., Lada, C. J., & Shu, F. H. 1987, ApJ, 312, 788 CrossRefGoogle Scholar
[3] Adams, F. C., Lada, C. J., & Shu, F. H. 1988, ApJ, 326, 865 CrossRefGoogle Scholar
[4] Basri, G., & Bertout, C. 1989, ApJ, 341, 340 CrossRefGoogle Scholar
[5] Beckwith, S., Sargent, A., Chini, R., & Gusten, R. 1990, AJ, 99, 1024 CrossRefGoogle Scholar
[6] Brooke, T.Y., Tokunaga, A.T., & Strom, S.E. 1993, AJ, in pressGoogle Scholar
[7] Hartmann, L., Kenyon, S.J., & Calvet, N. 1993, ApJ, 407, 219 CrossRefGoogle Scholar
[8] Hillenbrand, L.A., Strom, S.E., Vrba, F.J., & Keene, J. 1992, ApJ, 397, 613 CrossRefGoogle Scholar
[9] Kenyon, S. J., & Hartmann, L. 1987, ApJ, 323, 714 CrossRefGoogle Scholar
[10] Königl, A. 1991, ApJL 370, L39 CrossRefGoogle Scholar
[11] Lynden-Bell, & Pringle, 1974, MNRAS, 168, 603 CrossRefGoogle Scholar
[12] Lada, C.J., & Adams, F.C. 1992, ApJ, 393, 278 CrossRefGoogle Scholar
[13] Safier, P. 1993, ApJ, in pressGoogle Scholar
[14] Sellgren, K. 1984, ApJ, 277, 623 CrossRefGoogle Scholar
[15] Shu, F. H., Tremaine, S., Adams, F. C., & Ruden, S. P. 1990, ApJ, 358, 495 CrossRefGoogle Scholar
[16] Natta, A. 1993, ApJ, in pressGoogle Scholar
[17] Natta, A., Palla, F., Butner, H.M., Evans, N.J. II, Harvey, P.M. 1992, ApJ, 391, 805 CrossRefGoogle Scholar
[18] Natta, A., Palla, F., Butner, H.M., Evans, N.J. II, Harvey, P.M. 1993, ApJ, 406, 674 CrossRefGoogle Scholar
[19] Weintraub, D.A., Kastner, J.H., Zuckerman, B., & Gatley, I. 1992, ApJ, 391, 784 CrossRefGoogle Scholar
[20] Whitney, B. A., & Hartmann, L. 1993, ApJ, 402, 605 CrossRefGoogle Scholar
Beck, H.K.B., Gail, H.-P., Henkel, R., Sedlmayr, E., 1992, Astron. Astrophys., 265, 626 Google Scholar
Berriman, G.B., Reid, I.N., Leggett, S.K., 1992, Astrophys. J., 392, L31 CrossRefGoogle Scholar
Burrow, A., Liebert, J., 1993, Rev. Mod. Phys., 65, 301 CrossRefGoogle Scholar
Jørgensen, U.G.,(ed.), 1993, Proceedings of the 146-th IAU Colloquium on “Molecular Opacities in the Stellar Environment”, Lecture Notes in Physics, Springer-Verlag, in pressGoogle Scholar
Jørgensen, U.G., Johnson, H.R., 1992, Astron. Astrophys. 265, 168 Google Scholar
Jørgensen, U.G., Johnson, H.R., Nordlund, Å., 1992, Astron. Astrophys. 261, 263 Google Scholar
Keady, J.J., Ridgway, S.T., 1993, Astrophys. J., 406, 199 CrossRefGoogle Scholar
Kirkpatrick, J.D., Kelly, D.M., Rieke, G.H., Liebert, J., Allard, F., Wehrse, R., 1993, Astrophys. J., 402, 643 CrossRefGoogle Scholar
Lynas-Gray, A.E., Mendoza, C., Zeippen, C.J.,(ed), 1992. Proceedings of the Workshop on Astrophysical Opacities, in Rev. Mexicana Astron. Astrof., vol. 23, special issueGoogle Scholar
Plez, B., Brett, J.M. Nordlund, Å., 1992, Astron. Astrophys. 256, 551 Google Scholar
Rogers, B., Glassgold, A.E., 1991, Astrophys. J., 382, 606 CrossRefGoogle Scholar
Stevenson, D.J., 1991, Ann. Rev. Astron. Astrophys., 29, 163 CrossRefGoogle Scholar
Tinney, C.G., Mould, J.R., Reid, I.N., 1993, Astron. J., 105, 1045 CrossRefGoogle Scholar
Baschek, B., Papkalla, R., Wehrse, R. 1993, in: Proc. 2nd. Haifa Conf. on Cataclysmic Variables, Regev, O., Shaviv, G., eds.Google Scholar
Ben Jaffel, L., Vidal-Madjar, A. 1989, Astron. Astrophys. 220, 306 Google Scholar
Efstathiou, A., Rowan-Robinson, M. 1990, M.N.R.A.S. 245, 275 CrossRefGoogle Scholar
Führer, C. 1993, diploma thesis, Inst. f. Appl. Math., Heidelberg University Google Scholar
Johnson, C., Pitkâranta, J. 1983, SIAM J. Num. Anal. 20, 951 CrossRefGoogle Scholar
Jones, P.D., Bayazitoglu, Y. 1993, J.Q.R.S.T. 48, 427 Google Scholar
Langer, S.H., Ross, R.R., McCray, R. 1978, Astrophys. J. 222, 959 CrossRefGoogle Scholar
Myneni, R.B., Asrar, G., Gerstl, S.A.W. 1990, Transp. Theory St. Phys. 19, 205 CrossRefGoogle Scholar
Nordlund, Å. 1982, Astron. Astrophys. 107, 1 Google Scholar
Pozdnyakov, L.A., Sobol’, I.M., Sunyaev, R.A. 1983, Sov. Sci. Rev. (Sect. E) 2, 189.Google Scholar
Schiesser, W.E. 1991, The Numerical Method of Lines, Academic Press Google Scholar
Steffen, M., Freytag, B. 1991, Rev. Modern Astron. 4, 43 CrossRefGoogle Scholar
Stenholm, L.G., Storzer, H., Wehrse, R. 1991, J.Q.S.R.T. 45, 47 Google Scholar
Turek, S. 1993, Impact Comp. Sc. Eng., in pressGoogle Scholar
Turek, S., Wehrse, R. 1993, Astron. Astrophys. submittedGoogle Scholar