Abstract
The main problem for the interpretation of stellar spectral lines is to explain superionization and stellar winds. Results giving information on these two phenomena in solar-type stars, hot dwarfs and supergiants, A-type dwarfs and supergiants are reviewed.
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References
Abbott, D.C., Bohlin, R.C., Savage, B.D.: 1982, Astroph. J Suppl.48369.
Aydin, C. : 1972, Astron. Astroph.19 389.
Blanco, C., Catalano, S., Marilli, E.: 1980, 2nd IUE European Conference, ESA SP-157, p. 63
Borra, E.F., Landstreet, J.O.: 1979, Astroph. J.228 809.
Castor, J.I. : 1970, Mon. Not.149 111
Doazan, V. : 1982, in B Stars With and Without Emission Lines, NASA SP-456, p. 279.
Dravins, D. : 1982, Ann. Rev. Astron. Astroph.20 61
Evans, R.G., Jordan, C.: 1975, Mon. Not. 172 585
Felenbok, P., Praderie, F., Talavera, A.: 1983, Astron. Astroph.128 74.
Garmany, C.D. : 1982, in Observational Basis for Velocity Fields in Stellar Atmospheres, Ed. R. Stalio, Trieste-Workshop, p. 83.
Gray, D.F. : 1982, Mem. Soc. Astron. It.53 931
Gry, C. Lamers, H.J.G.L.M., Vidal-Madjar, A.: 1984, Astron. Astroph.137 29
Hartmann, L., Baljunas, S.L., Duncan, D.K., Noyes, R.W.: 1984, Astroph. J.279 778.
Hack, M., Selvelli, P.L.: 1979, Astron. Astroph.75 316.
Kondo, Y., Morgan, T.H., Modisette, J.L.: 1977, Astron. Soc. Pacific89 675.
Lamers, H.J.G.L.M., Gathier, R., Snow, T.P.: 1982, Astroph. J.258 186.
Livingston, W.C. : 1983, in Solar and Stellar Magnetic Fields: Origins and Coronal Effects, IAU Symp. No. 102, J. Stenflo ed.
Lucy, L.B. : 1982, Astroph. J.255 278
Lucy, L.B. : 1982, Astroph. J.255 286
Marcy, G.W. : 1981, Astroph. J.245624.
Molaro, P., Morossi, C., Ramella, M., Franco, M.: 1983, Astron. Astroph.127 L3
Molaro, P. Morossi, C., Ramella, M., Franco, M. 1984, 4 th IUE European Conference, ESA-SP 218, p. 223.
Noyes, R.W., Hartmann, L.W., Baljunas, S.L., Duncan, D.K., Vaughan, A.H.: 1984, Astroph. J.279 763.
Praderie, F., Lamers, H.J.G.L.M., Talavera, A.: 1980, Astron. Astroph.86 271
Robinson, R.D., Worden, S.P., Harvey, J.W.: 1980, Astroph. J. Lett.236 L155.
Simon, T. : 1984, Astroph. J.279 738
Slettebak, A., Carpenter, K. G.: 1983, Astroph. J. Suppl.53 869.
Smith, M.A., Karp, A.H.: 1978, Astroph. J.219 522.
Smith, M.A., Karp, A.H.: 1978, Astroph. J.230 156.
Snow, T.P., Morton, D.C.: 1976, Astroph. J. Suppl.32429
Tjin A Djie, H.R.E., Thé, P.S., Hack, M., Selvelli, P.L.: 1982, Astron. Astroph.106 98.
Underhill, A.B. : 1983, Astroph. J.265 933
Underhill, A.B., Fahey, R.P.: 1984, Astroph. J.280 712.
Willis, A.J. : 1982, in Observational Basis for Velocity fields in Stellar Atmospheres, Ed. R. Stalio, Trieste-Workshop, p. 111.
Zwaan, C. : 1977, Mem. Soc. Astron. It.48 525.
Zwaan, C. : 1981, in Solar Phenomena in Stars and Stellar systems eds. R.M. Bonnet, A.K. Dupree, Reidel, Dordrecht, p. 463
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© 1985 D. Reidel Publishing company,Dordrecht, Holland
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Hack, M. (1985). Observational Problems in Spectral Line Formation. In: Beckman, J.E., Crivellari, L. (eds) Progress in Stellar Spectral Line Formation Theory. NATO ASI Series, vol 152. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-5372-7_22
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DOI: https://doi.org/10.1007/978-94-009-5372-7_22
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