Transition probabilities of astrophysical interest in the niobium ions Nb+ and Nb2+

Astronomy and Astrophysics

Volumn 511, Issue 2, 2010, Pages

  Nilsson, H ^a   Hartman, H ^a   Engstrom L ^b   Lundberg, H ^b   Sneden, C ^c   Fivet, V ^d   Palmeri, P ^d   Quinet, P ^d,e   Biemont E I ^d,e  

^a LUND UNIVERSITY   (Sweden)

^b LUND UNIVERSITY   (Sweden)

^c UNIVERSITY OF TEXAS AT AUSTIN   (United States)

^d UNIVERSITY OF MONS   (Belgium)

^e UNIVERSITY OF LIÈGE   (Belgium)

Author keywords

Atomic data; Atomic processes; Stars: abundances; Sun: abundances

Indexed keywords

ATOMS; NIOBIUM; PROBABILITY; SPECTROSCOPY; SUN;

ABUNDANCE RATIOS; ATOMIC DATA; ATOMIC PROCESS; BRANCHING FRACTIONS; CORE POLARIZATION; FOURIER TRANSFORM SPECTROSCOPY; HYPERFINES; LABORATORY MEASUREMENTS; METAL-POOR STAR; NIOBIUM IONS; PRODUCTION METHODS; R-PROCESS; RADIATIVE LIFETIME; RELATIVISTIC HARTREE-FOCK METHODS; SPECTRAL LINE; STARS: ABUNDANCES; SYNTHETIC SPECTRA; TIME-RESOLVED LASER-INDUCED FLUORESCENCE; TRANSITION PROBABILITIES; TRANSITION PROBABLITIES; WAVELENGTH REGIONS;

STARS;

EID: 77950385251     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913574     Document Type: Article

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