J/A+A/434/365   A-values & oscillator strength of O-like ions (Landi+, 2005)

Radiative transition probabilities in the O-like sequence. Landi O. <Astron. Astrophys. 434, 365 (2005)> =2005A&A...434..365L 2005A&A...434..365L
ADC_Keywords: Atomic physics Keywords: atomic data - atomic processes - radiation mechanisms: general - line: formation - Sun: corona Abstract: In the present work a complete set of radiative transition rates is calculated for all for the O-like ions with Z=11-30. Energy levels, oscillator strengths and A values are computed for all transitions within the n=2 complex and are compared with previous calculations, where available. Calculations are carried out using the Superstructure code. The present work provides for the first time a self-consistent, complete set of A values necessary for the calculation of line emissivities and synthetic spectra for all the ions considered, filling several gaps in the existing literature. The present data are especially suited for the analysis of spectral lines emitted by the less-abundant elements in the universe, for which few if any data were available in the literature. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 53 200 Energies for the n=2 levels in the O-like isoelectronic sequence aos.dat 39 780 A-values and weighted oscillator strengths for the O-like sequence (tables 3-8 of the paper) -------------------------------------------------------------------------------- See also: VI/72 : Atomic Transition Probabilities, Sc-Ni (NIST 1993) J/A+A/385/716 : N-like and O-like Breit-Pauli energy levels (Tachiev+, 2002) J/A+AS/108/1 : IRON Project. V. O-like ions (Butler+, 1994) Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Ion Ion designation 10- 11 I2 --- Index Index number 13- 23 A11 --- Level Level designation 24- 33 F10.2 cm-1 E Experimental energy (1) 38- 47 F10.2 cm-1 Eth Theoretical energy calculated in the present work -------------------------------------------------------------------------------- Note (1): Experimental energies come from Edlen (1983, Phys. Scr. 28, 51), with the only exception of Fe XIX and Ni XXI, which are taken from Shirai et al. (2000, J. Phys. Chem. Ref. Data Monograph, 8). -------------------------------------------------------------------------------- Byte-by-byte Description of file: aos.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 8 A8 --- Ion Ion designation 10 I1 --- Down Lower level index 12 A1 -- --- [-] 14- 15 I2 --- Up Upper level index 17- 19 A3 --- Type Type of transition (1) 21- 29 E9.4 s-1 A A-value 31- 39 E9.4 --- gf Weighted oscillator strength -------------------------------------------------------------------------------- Note (1): Type of transition as follows: E1 = electric dipole transitions E1f = spin-forbidden E1 transitions E2 = electric quadrupole transitions M1 = magnetic dipole transitions M2 = magnetic quadrupole transitions. -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Patricia Vannier [CDS] 04-Apr-2005
The document above follows the rules of the Standard Description for Astronomical Catalogues; from this documentation it is possible to generate f77 program to load files into arrays or line by line