Abstract
Results of computations of the statistical equilibrium of lithium in dwarf atmospheres of Teff = 6270, 5770, 5270 K, log g= 4.44 and [m/H] = −0, −1, −2, −3 are discussed. It is shown that NLTE corrections are less than 0.1 dex for abundances of lithium observed in halo dwarfs.
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References
Auer,R.N., Heasley,I.N., 1976, Ap. J., 205, 165.
Holweger,H., Muller, E. A. Solar physics, 1974, 9, 19. Ni
Kurucz R.L., 1975, SAO Special report N 309
Kurucz R.L., Peytremann, E.A, 1975, SAO Special report N 362.
Lambert, D.L., Physica Scripta, 1993, T47, 186
Maltby, P., Avrett, E.H., Carlsson, M., Kjeldseth-Moe, O., Kurucz, R., L., Leser R. Ap. J., 1986, 306, 284.
Magazzu, A., Rebolo, R., Pavlenko, Ya.V., 1993, Ap. J., 292, 159.
Pavlenko Ya.V., 1990, Kinemat. i fizika nebes. tel, 6, 58
Pavlenko Ya.V. Soy. Astron., 1994, in press.
Peytremann, 1974, A&A 203, 33
Rebolo, R., Molaro P., Beckman, J.E A&A, 1988, 192, 192.
Rutten R.J., Kostik R.I. A& A, 1982, 115, 104.
Spite F., Spite M., 1982, A& A, 115, 337.
Steenbock, W., Holweger H., 1984, A&A, 130, 319
Wiese, W.L., Smith, M.W., Glennon,B.M., 1966, Atomic lines probabilities NSRD-NBS 41
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© 1995 Springer-Verlag Berlin Heidelberg
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Pavlenko, Y.V. (1995). Li I Lines in POP II Dwarf Spectra: NLTE Effects. In: Crane, P. (eds) The Light Element Abundances. ESO Astrophysics Symposia. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-540-49169-9_54
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DOI: https://doi.org/10.1007/978-3-540-49169-9_54
Publisher Name: Springer, Berlin, Heidelberg
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