[en] Selective lifetime measurements by time-resolved laser-induced fluorescence spectroscopy for 5 levels belonging to the 4f(3)5d configuration of doubly ionized neodymium provide a first and useful experimental test of the relativistic Hartree-Fock calculations in this ion of astrophysical interest. As a consequence, the accuracy of the transition probabilities deduced in the present work is well assessed. These new data are expected to help astrophysicists in the future to refine the analysis of the composition of chemically peculiar stars which frequently show large overabundances of lanthanides when compared to the solar system standards.
Disciplines :
Earth sciences & physical geography
Author, co-author :
Zhang, Z. G.
Svanberg, S.
Palmeri, P.
Quinet, Pascal ; Université de Liège - ULiège > Département de physique > Physique nucléaire, atomique et spectroscopie
Biémont, Emile ; Université de Liège - ULiège > Département de physique > Physique nucléaire, atomique et spectroscopie
Language :
English
Title :
Measurement of lifetimes by laser-induced fluorescence and determination of transition probabilities of astrophysical interest in NdIII
Biémont E., Li Z.S., Palmeri P., Quinet P. J. Phys. B 1999, 32:3409.
Biémont E., Garnir H.P., Bastin T. MNRAS 2001, 321:481.
Biémont E., Garnir H.P., Palmeri P. Phys. Rev. 2001, 64:022503.
Biémont E., Garnir H.P., Li Z.S. J. Phys. B 2001, 34:1869.
Biémont E., Palmeri P., Quinet P. MNRAS 2001, 328:1085.
Bord D.J. A&A 2000, 144:517.
Brewer J. JOSA 1971, 59:2083.
Cowan R.D. The Theory of Atomic Structure and Spectra, (University of California Press, Berkeley, CA, USA); 1981.
Cowley C.R. ApJS 1976, 32:631.
Cowley C.R. Phys. Scr. 1984, T8:28.
Cowley C.R., Bord D.J. The Third Spectrum of Neodymium: Application to HR 6870 and γEquulei, in The Scientific Impact of the Goddard High Resolution Spectrograph , ed. J. C. Brandt, T. B. Ake III, C. C. Petersen, ASP Conf. Ser.; 1998, 143:346.
Cowley C.R., Crosswhite H.M. PASP 1978, 90:108.
Cowley C.R., Bidelman W.P., Mathys G. BAAS 1998, 30:1317.
Cowley C.R., Greenberg M. MNRAS 1988, 232:763.
Cowley C.R., Ryabchikova T., Kupka F. MNRAS 2000, 317:299.
Crosswhite H., 1976, unpublished work, quoted by Martin et al.; 1975.
Hensberge H., Van Santvoort J., Van Der Hucht K.A., Morgan T.H. A&A 1986, 158:113.
Jaschek C., Jaschek M. The Behavior of Chemical Elements in Stars, (Cambridge University Press); 1995.
Lambert D.L. Cool Stars in Excesses of Heavy Elements , ed. M. Jaschek, & P. C. Keenan (Reidel); 1985, 191.
Leckrone D.S. The Physics of Ap Stars, IAU Colloq. 32, ed. W. W. Weiss, H. Jenkner, & J. J. Wood, Universitätssterwarte Wien, Vienna; 1976.
Leckrone D.S., Proffitt C.R., Wahlgren G.M., Johansson S.G., Brage T. AJ 1999, 117:1454.
Li Z.S., Lundberg H., Wahlgren G.M., Sikström C.M. Phys. Rev. A , Electronic version Ref. No. 032505; 2000, 62.
Li Z.S., Zhang Z.G., Lokhnygin V. J. Phys. B 2001, 34:1349.
Li Z.S., Jiang Z.K. Phys. Scr. 1999, 60:414.
Martin W.C., Zalubas R., Hagan L. Atomic Energy Levels, The Rare-Earth Elements, Nat. Bur. Stand. Ref. Data Ser. 60, Washington D.C., USA; 1978.
Merrill P.W. Lines of the Chemical Elements in Astronomical Spectra , Carnegie Institute of Washington, Publ.; 1956, 610.