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相关论文: Experimental Ti I oscillator strengths and their a…

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We report new experimental Fe I oscillator strengths obtained by combining measurements of branching fractions measured with a Fourier Transform spectrometer and time-resolved laser-induced fluorescence lifetimes. The study covers the…

太阳与恒星天体物理 · 物理学 2017-11-01 M. T. Belmonte , J. C. Pickering , M. P. Ruffoni , E . A. Den Hartog , J. E. Lawler , A. Guzman , U. Heiter

This work reports new experimental radiative lifetimes and calculated oscillator strengths for transitions of astrophysical interest in singly ionized cobalt. More precisely, nineteen radiative lifetimes in Co+ have been measured with the…

太阳与恒星天体物理 · 物理学 2016-10-02 P. Quinet , V. Fivet , P. Palmeri , L. Engstrom , H. Hartman , H. Lundberg , H. Nilsson

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…

太阳与恒星天体物理 · 物理学 2017-04-12 H. Hartman , L. Engstrom , H. Lundberg , H. Nilsson , P. Quinet , V. Fivet , P. Palmeri , G. Malcheva , K. Blagoev

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…

太阳与恒星天体物理 · 物理学 2015-06-23 E. A. Den Hartog , M. P. Ruffoni , J. E. Lawler , J. C. Pickering , K. Lind , N. R. Brewer

We present lifetime measurements using beam-foil techniques for radiative transitions from the 3$p^4$($^1S$)4$s$ $^2S_{1/2}$, 3$p^4$($^3P$)5$s$ $^2P_{1/2,3/2}$, and 3$p^4$($^3P$)3$d$ $^2F_{5/2}$ levels in Cl I and the corresponding results…

原子物理 · 物理学 2020-01-08 R. B. Alkhayat , R. E. Irving , S. R. Federman , D. G. Ellis , S. Cheng

We report calculations of energy levels, radiative rates, oscillator strengths and line strengths for transitions among the lowest 345 levels of Ti X. These include 146 levels of the $n \le$ 3 configurations and 86 of 3s$^2 4\ell$, 3s$^2…

原子物理 · 物理学 2013-07-11 KM Aggarwal , FP Keenan

We report experimental oscillator strengths for 28 infrared Fe I transitions, for which no previous experimental values exist. These transitions were selected to address an urgent need for oscillator strengths of lines in the H-band…

太阳与恒星天体物理 · 物理学 2015-06-17 M. P. Ruffoni , J. C. Pickering , C. Allende Prieto , G. Nave

The lifetimes of 17 even-parity levels (3d5s, 3d4d, 3d6s, and 4p$^2$) in the region 57743-77837 cm$^{-1}$ of singly ionised scandium (\ion{Sc}{ii}) were measured by two-step time-resolved laser induced fluorescence spectroscopy. Oscillator…

太阳与恒星天体物理 · 物理学 2017-08-23 A. Pehlivan Rhodin , M. T. Belmonte , L. Engstrom , H. Lundberg , H. Nilsson , H. Hartman , J. C. Pickering , C. Clear , P. Quinet , V. Fivet , P. Palmeri

We report on calculations of energy levels, radiative rates, oscillator strengths, and line strengths for transitions among the lowest 253 levels of the (1s$^2$2s$^2$2p$^6$) 3s$^2$3p$^5$, 3s3p$^6$, 3s$^2$3p$^4$3d, 3s3p$^5$3d,…

原子物理 · 物理学 2013-07-10 KM Aggarwal , FP Keenan , AZ Msezane

Elemental abundances can be determined from stellar spectra, making it possible to study galactic formation and evolution. Accurate atomic data is essential for the reliable interpretation and modeling of astrophysical spectra. In this…

太阳与恒星天体物理 · 物理学 2023-09-13 Madeleine Burheim , Henrik Hartman , Hampus Nilsson

Lifetime measurements using beam foil techniques for the $5s5p^{2}$ $^{2}D_{3/2,5/2}$ levels in Sn II are presented. The resulting oscillator strengths for transitions at 1699.4, 1831.8 and 1811.2 \AA{} are reported. We also studied these…

原子物理 · 物理学 2016-10-19 N Heidarian , R E Irving , S R Federman , D G Ellis , S Cheng , L J Curtis

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…

太阳与恒星天体物理 · 物理学 2015-05-14 J. Gurell , H. Nilsson , L. Engstrom , H. Lundberg , R. Blackwell-Whitehead , K. E. Nielsen , S. Mannervik

Context. Atomic data is crucial for astrophysical investigations. To understand the formation and evolution of stars, we need to analyse their observed spectra. Analysing a spectrum of a star requires information about the properties of…

天体物理仪器与方法 · 物理学 2015-10-21 A. Pehlivan , H. Nilsson , H. Hartman

We report calculations of energy levels, radiative rates, oscillator strengths and line strengths for transitions among the lowest 231 levels of Ti VII. The general-purpose relativistic atomic structure package ({\sc grasp}) and flexible…

太阳与恒星天体物理 · 物理学 2015-06-17 KM Aggarwal , FP Keenan

The stellar abundance ratio of Mg/Fe is an important tool in diagnostics of galaxy evolution. In order to make reliable measurements of the Mg abundance of stars, it is necessary to have accurate values for the oscillator strength (f-value)…

天体物理学 · 物理学 2009-11-11 M. Aldenius , J. D. Tanner , S. Johansson , H. Lundberg , S. G. Ryan

Branching fractions were measured for electric dipole transitions from the 5p upper levels to the 5s levels in neutral krypton atoms. The measurements were made with a wall-stabilized electric arc and a 2m monochromator for the spectral…

原子物理 · 物理学 2009-11-06 Krzysztof Dzierzega , Udo Volz , Gillian Nave , Ulf Griesmann

Band oscillator strengths for electronic transitions in CO were obtained at the Synchrotron Radiation Center of the University of Wisconsin-Madison. Our focus was on transitions that are observed in interstellar spectra with the Far…

天体物理学 · 物理学 2009-11-06 S. R. Federman , M. Fritts , S. Cheng , K. M. Menningen , David C. Knauth , K. Fulk

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…

太阳与恒星天体物理 · 物理学 2018-10-10 J. E. Lawler , T. Feigenson , C. Sneden , J. J. Cowan , G. Nave

Energies and lifetimes are reported for the lowest 136 levels of Fe XIV, belonging to the (1s$^2$2s$^2$2p$^6$) 3s$^2$3p, 3s3p$^2$, 3s$^2$3d, 3p$^3$, 3s3p3d, 3p$^2$3d, 3s3d$^2$, 3p3d$^2$ and 3s$^24\ell$ configurations. Additionally,…

太阳与恒星天体物理 · 物理学 2015-06-22 K M Aggarwal , F P Keenan

We have studied possible candidates for laser cooling transitions in $^{169}$Tm in the spectral region 410 -- 420 nm. By means of saturation absorption spectroscopy we have measured the hyperfine structure and rates of two nearly closed…

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