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Related papers: Hf Transition Probabilities and Abundances

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We report new branching fraction measurements for 199 UV and optical transitions of Hf II. These transitions range in wavelength (wavenumber) from 2068- 6584 A (48322-15183 cm-1) and originate in 17 odd-parity upper levels ranging in energy…

Solar and Stellar Astrophysics · Physics 2021-05-05 E. A. Den Hartog , J. E. Lawler , I. U. Roederer

Recent radiative lifetime measurements accurate to +/- 5% (Stockett et al. 2007, J. Phys. B 40, 4529) using laser-induced fluorescence (LIF) on 8 even-parity and 62 odd-parity levels of Er II have been combined with new branching fractions…

Recent radiative lifetime measurements accurate to +/- 5% using laser-induced fluorescence (LIF) on 43 even-parity and 15 odd-parity levels of Ce II have been combined with new branching fractions measured using a Fourier transform…

Solar and Stellar Astrophysics · Physics 2009-11-13 J. E. Lawler , C. Sneden , J. J. Cowan , I. I. Ivans , E. A. Den Hartog

Radiative lifetimes, accurate to +/- 5%, have been measured for 49 even-parity and 14 odd-parity levels of Gd II using laser-induced fluorescence. The lifetimes are combined with branching fractions measured using Fourier transform…

Astrophysics · Physics 2007-05-23 E. A. Den Hartog , J. E. Lawler , C. Sneden , J. J. Cowan

Radiative lifetimes, accurate to +/- 5%, have been measured for 212 odd-parity levels of Sm II using laser-induced fluorescence. The lifetimes are combined with branching fractions measured using Fourier-transform spectrometry to determine…

Astrophysics · Physics 2007-05-23 J. E. Lawler , E. A. Den Hartog , C. Sneden , J. J. Cowan

Fe II radiative lifetimes were measured applying the time-resolved nonlinear laser-induced fluoresence technique. We investigated 21 levels of up to 47000 1/cm. The uncertainties are typically 2-3%. The lifetimes provide an improved…

Astrophysics · Physics 2009-11-10 R. Schnabel , M. Schultz-Johanning , M. Kock

New branching fraction measurements based primarily on data from a cross dispersed echelle spectrometer are reported for 84 lines of Co II. The branching fractions for 82 lines are converted to absolute atomic transition probabilities using…

Solar and Stellar Astrophysics · Physics 2018-10-10 J. E. Lawler , T. Feigenson , C. Sneden , J. J. Cowan , G. Nave

Atomic transition probability measurements for 364 lines of Ti II in the UV through near IR are reported. Branching fractions from data recorded using a Fourier transform spectrometer and a new echelle spectrometer are combined with…

Solar and Stellar Astrophysics · Physics 2014-02-19 M. P. Wood , J. E. Lawler , C. Sneden , J. J. Cowan

Branching fraction measurements from Fourier transform spectra in conjunction with published radiative lifetimes are used to determine transition probabilities for 263 lines of neutral chromium. These laboratory values are employed to…

Astrophysics · Physics 2009-11-13 Jennifer S. Sobeck , James E. Lawler , Christopher Sneden

New experimental absolute atomic transition probabilities are reported for 203 lines of V II. Branching fractions are measured from spectra recorded using a Fourier transform spectrometer and an echelle spectrometer. The branching fractions…

Solar and Stellar Astrophysics · Physics 2015-06-22 M. P. Wood , J. E. Lawler , E. A. Den Hartog , C. Sneden , J. J. Cowan

We present abundances for Ru and Hf, compare them to abundances of other heavy elements, and discuss the problems found in determining Ru and Hf abundances with laboratory gf-values in the spectra of barium stars. We determined Ru and Hf…

Astrophysics · Physics 2009-11-13 D. M. Allen , G. F. Porto de Mello

We report new branching fraction measurements for 156 ultraviolet and optical transitions of Gd II. These transitions range in wavelength (wavenumber) from 2574 to 6766 Angstroms (38838 - 14777 cm-1) and originate in one odd-parity and 11…

Solar and Stellar Astrophysics · Physics 2025-03-31 G. T. Voith , E. A. Den Hartog , I. U. Roederer

Aims: We measure transition probabilities for Cr II transitions from the z ^4H_J, z ^2D_J, y ^4F_J, and y ^4G_J levels in the energy range 63000 to 68000 cm^{-1}. Methods: Radiative lifetimes were measured using time-resolved laser-induced…

Solar and Stellar Astrophysics · Physics 2015-05-14 J. Gurell , H. Nilsson , L. Engstrom , H. Lundberg , R. Blackwell-Whitehead , K. E. Nielsen , S. Mannervik

We report new branching fractions for 121 UV lines from the low-lying odd-parity levels of Fe II belonging to the z6Do, z6Fo, z6Po, z4Fo, z4Do and z4Po terms of the 3d6(5D)4p configuration. These lines range in wavelength from 2250 - 3280…

Solar and Stellar Astrophysics · Physics 2019-08-21 E. A. Den Hartog , J. E. Lawler , C. Sneden , J. J. Cowan , A. Brukhovesky

We report new branching fraction measurements for 224 ultraviolet (UV) and optical transitions of Tm II. These transitions range in wavelength (wavenumber) from 2350 - 6417 Angstroms (42532 - 15579 cm-1) and originate in 13 odd-parity and…

Solar and Stellar Astrophysics · Physics 2024-07-24 E. A. Den Hartog , G. T. Voith , I. U. Roederer

Atomic transition probability measurements for 371 Ni I lines in the UV through near IR are reported. Branching fractions from data recorded using a Fourier transform spectrometer and a new echelle spectrograph are combined with published…

Solar and Stellar Astrophysics · Physics 2014-03-28 M. P. Wood , J. E. Lawler , C. Sneden , J. J. Cowan

We report new measurements of branching fractions for 20 UV and blue lines in the spectrum of neutral silicon (Si I) originating in the 3$s^{2}$3$p$4$s$ $^{3}$P$^{\rm o}_{1,2}$, $^{1}$P$^{\rm o}_{1}$ and 3$s$3$p^{3}$ $^{1}$D$^{\rm o}_{1,2}$…

Solar and Stellar Astrophysics · Physics 2023-03-29 E. A. Den Hartog , J. E. Lawler , C. Sneden , I. U. Roederer , J. J. Cowan

Abundances of heavier elements (barium and beyond) in many neutron-capture-element-rich halo stars accurately replicate the solar system r-process pattern. However, abundances of lighter neutron-capture elements in these stars are not…

The available data for E2 transition strengths in the region between neutron-deficient Hf and Pt isotopes are far from complete. More and precise data are needed to enhance the picture of structure evolution in this region and to test…

This work reports new experimental radiative lifetimes and calculated oscillator strengths for transitions from 3d8 4d levels of astrophysical interest in singly ionized nickel. Radiative lifetimes of seven high-lying levels of even parity…

Solar and Stellar Astrophysics · Physics 2017-04-12 H. Hartman , L. Engstrom , H. Lundberg , H. Nilsson , P. Quinet , V. Fivet , P. Palmeri , G. Malcheva , K. Blagoev
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