Voir la notice du chapitre de livre
Mots-clés : non-LTE calculations
@article{UZKU_2011_153_2_a11,
author = {U. Sh. Bayazitov},
title = {On the abundance of iron and zinc in metal-poor stars},
journal = {U\v{c}\"enye zapiski Kazanskogo universiteta. Seri\^a Fiziko-matemati\v{c}eskie nauki},
pages = {108--114},
year = {2011},
volume = {153},
number = {2},
language = {ru},
url = {http://geodesic.mathdoc.fr/item/UZKU_2011_153_2_a11/}
}
TY - JOUR AU - U. Sh. Bayazitov TI - On the abundance of iron and zinc in metal-poor stars JO - Učënye zapiski Kazanskogo universiteta. Seriâ Fiziko-matematičeskie nauki PY - 2011 SP - 108 EP - 114 VL - 153 IS - 2 UR - http://geodesic.mathdoc.fr/item/UZKU_2011_153_2_a11/ LA - ru ID - UZKU_2011_153_2_a11 ER -
U. Sh. Bayazitov. On the abundance of iron and zinc in metal-poor stars. Učënye zapiski Kazanskogo universiteta. Seriâ Fiziko-matematičeskie nauki, Uchenye Zapiski Kazanskogo Universiteta. Seriya Fiziko-Matematicheskie Nauki, Tome 153 (2011) no. 2, pp. 108-114. http://geodesic.mathdoc.fr/item/UZKU_2011_153_2_a11/
[1] Sneden C., Gratton R. G., Crocker D. A., “Trend in copper and zinc abundances for disc and halo stars”, Astron. Astrophys., 246:2 (1991), 354–367
[2] Mishenina T. V., Kovtyukh V. V., Soubiran C., Travaglio C., Busso M., “Abundances of Cu and Zn in metal-poor stars: Clues for Galaxy evolution”, Astron. Astrophys., 396:1 (2002), 189–201 | DOI
[3] Bayazitov U. Sh., Thevenin F., “About trend in zinc stellar abundances with metallicity”, Odessa Astron. Publ., 20:1 (2007), 12–15
[4] Kurucz R. L., “A new opacity-sampling model atmosphere program for arbitrary abundances. Presented at IAU Colloquium 138”, Peculiar versus Normal Phenomena in A-type and Related Stars, A.S.P. Conf. Ser., 44, eds. M. M. Dworetsky, F. Castelli, R. Faraggiana, 1993, 87–97
[5] Nave G., Johansson S., Learner R., Thorn A., Brault J., “A new multiplet table for Fe I”, Astrophys. J. Suppl. Ser., 94:1 (1994), 221–459 | DOI
[6] van Regemorter H., “Rate of collisional excitation in stellar atmospheres”, Astrophys. J., 136 (1962), 906–915 | DOI
[7] Allen K. U., Astrofizicheskie velichiny, Mir, M., 1977, 446 pp.
[8] Siton M., Atomnye i molekulyarnye protsessy, Mir, M., 1963, 777 pp.
[9] Steenbock W., “Statistical equilibrium of Fe I/Fe II in cool stars”, Cool stars with excesses of heavy elements, Reidel, Dordrecht, 1997, 231–235
[10] Bautista M., “Atomic data from the IRON Project. XX. Photoionization cross-sections and oscillator strengths for Fe I”, Astron. Astrophys. Suppl. Ser., 122 (1997), 167–176 | DOI
[11] Bayazitov U. Sh., “On the effect of line blanketing on the Fe I line intensities in the solar, Arcturus and Procyon spectra”, Astron. Astrophys. Trans., 22:6 (2003), 855–859 | DOI
[12] Grei D., Nablyudenie i analiz zvezdnykh atmosfer, Mir, M., 1980, 496 pp.
[13] Anstee S. D., O'Mara B. J., Ross J. E., “A determination of the solar abundance of iron from the strong lines of Fe I”, Mon. Not. R. Astron. Soc., 284:1 (1997), 202–212 | DOI
[14] Carlsson M., A computer program for solving multi-level non-LTE radiative transfer problems in moving or static atmospheres, Rep. No 33, Upps. Astron. Obs., Uppsala, 1986, 165 pp., svobodnyi URL: http://folk.uio.no/matsc/mul22/report33.pdf
[15] Cayrel R., Depagne E., Spite M., Hill V., Spite F., Francois P., Plez B., Beers T., Primas F., Andersen J., Barbuy B., Bonifacio P., Molaro P., Nordstrom B., “First stars V – Abundance patterns from C to Zn and supernova yields in the early Galaxy”, Astron. Astrophys., 416:3 (2004), 1117–1138 | DOI
[16] Nissen P. E., Akerman C., Asplund M., Fabbian D., Kerber F., Kaufl H. U., Pettini M., “Sulphur and zinc abundances in Galactic halo stars revisited”, Astron. Astrophys., 469:1 (2007), 319–330 | DOI
[17] Boyarchuk A. A., Lyubimkov L. S., Sakhibullin N. A., “Effekty otkloneniya ot LTR v atmosferakh F-gigantov. Povyshenie ionizatsii atomov Fe I”, Astrofizika, 22 (1985), 339–356