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Related papers: Gd Transition Probabilities and Abundances

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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

Radiative lifetimes from laser-induced fluorescence measurements, accurate to about +/- 5 percent, are reported for 41 odd-parity levels of Hf II. The lifetimes are combined with branching fractions measured using Fourier transform…

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

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

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…

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

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

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

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

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

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

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

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

We report lifetime measurements of the 6 levels in the 3d6(5D)4d e6G term in Fe ii at an energy of 10.4 eV, and f -values for 14 transitions from the investigated levels. The lifetimes were measured using time-resolved laser-induced…

Solar and Stellar Astrophysics · Physics 2016-10-31 H. Hartman , H. Nilsson , L. Engström , H. Lundberg

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

The rapid neutron-capture process, creating about half of the heaviest elements in the Solar System was believed to be unique. Many recent studies have shown that this does not include the formation of lighter elements (in particular 38 < Z…

We study the solar photospheric abundance of singly ionized neodymium (Nd II) using high resolution spectroscopic data obtained by Fourier transform spectrograph (FTS). Based on the Local Thermodynamical Equilibrium (LTE) assumption, a new…

Solar and Stellar Astrophysics · Physics 2017-12-20 A. G. A. Abdelkawy , Abdelrazek M. K. Shaltout , M. M. Beheary , A. Bakry

Lanthanide elements play important roles as an opacity source in the ejected material from neutron star mergers. Accurate and complete atomic data are necessary to evaluate the opacities and to analyze the observed data. In this paper, we…

Atomic Physics · Physics 2020-05-13 Laima Radžiūtė , Gediminas Gaigalas , Daiji Kato , Pavel Rynkun , Masaomi Tanaka

Accurate transition probabilities for forbidden lines are important diagnostic parameters for low-density astrophysical plasmas. In this paper we present experimental atomic data for forbidden [FeII] transitions that are observed as strong…

Solar and Stellar Astrophysics · Physics 2015-05-14 J. Gurell , H. Hartman , R. Blackwell-Whitehead , H. Nilsson , E. Backstrom , L. O. Norlin , P. Royen , S. Mannervik

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

New radiative lifetimes, measured to $\pm$ 5 % accuracy, are reported for 31 even-parity levels of Fe I ranging from 45061 cm$^{-1}$ to 56842 cm$^{-1}$. These lifetimes have been measured using single-step and two-step time-resolved…

Solar and Stellar Astrophysics · Physics 2015-06-23 E. A. Den Hartog , M. P. Ruffoni , J. E. Lawler , J. C. Pickering , K. Lind , N. R. Brewer
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