J/A+A/529/A147 Photoionization cross sections of Selenium ions (Sterling+, 2011)

Atomic data for neutron-capture elements. I. Photoionization and recombination properties of low-charge selenium ions. Sterling N.C., Witthoeft M.C. <Astron. Astrophys. 529, A147 (2011)> =2011A&A...529A.147S 2011A&A...529A.147S
ADC_Keywords: Atomic physics Keywords: atomic data - atomic processes - HII regions - nucleosynthesis, abundances - planetary nebulae: general - stars: evolution Abstract: We present multi-configuration Breit-Pauli AUTOSTRUCTURE calculations of distorted-wave photoionization (PI) cross sections, and total and partial final-state resolved radiative recombination (RR) and dielectronic recombination (DR) rate coefficients for the first six ions of the trans-iron element Se. These calculations were motivated by the recent detection of Se emission lines in a large number of planetary nebulae. Se is a potentially useful tracer of neutron-capture nucleosynthesis, but accurate determinations of its abundance in photoionized nebulae have been hindered by the lack of atomic data governing its ionization balance. Our calculations were carried out in intermediate coupling with semi-relativistic radial wavefunctions. PI and recombination data were determined for levels within the ground configuration of each ion, and experimental PI cross-section measurements were used to benchmark our results. For DR, we allowed Δn=0 core excitations, which are important at photoionized plasma temperatures. Description: 'Direct' and 'Direct and resonant' photoionization cross sections are tabulated for neutral and the first five ions of Se. Note that photoexcitation-autoionization resonances are not included in these data files. Names of the files are given by pxd.dat (px.dat), e.g., se2+pxd.dat (se2+px.dat) for photoionization of Se2+ ions. Comments are indicated by '#' in the first column of a line. The first two lines of a file are header information indicating the number of photon targets (ground state and metastable states in the ground configuration, with 1 the lowest energy) and number of energies. The photoionization cross section of each state is preceded by a comment giving the energy above the ground state (or the total energy, in the case of the ground state), the total energy of the target state, and the energy-order of that state (1 = ground state, 2 = first excited state, etc.). All energies are reported in Rydbergs, and cross sections in megabarns (10-18cm2). Total and partial final state resolved dielectronic recombination rate coefficients are tabulated for the first six ions of Se, in the ADAS adf09 and adf48 formats. Names of the files are given by adf09_.dat (adf48_), e.g., adf09_se2+.dat (adf48_se2+.dat) gives dielectronic recombination data for Se2+ forming Se+. These files are available in adf subdirectory. The format of these files is complex, and beyond the scope of this README file. The reader is referred to http://amdpp.phys.strath.ac.uk/tamoc/RR/RR_web/appxa-09.pdf for a complete description of the adf09 and adf48 files format. File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table1.dat 223 21 Configuration-interaction expansions used for each Se ion se0_pxd.dat 30 225005 Direct Se0 photoionization cross section se1_pxd.dat 30 225005 Direct Se+ photoionization cross section se2_pxd.dat 30 225005 Direct Se2+ photoionization cross section se3_pxd.dat 30 180004 Direct Se3+ photoionization cross section se4_pxd.dat 30 45001 Direct Se4+ photoionization cross section se5_pxd.dat 30 45001 Direct Se5+ photoionization cross section se0_px.dat 78 292046 Direct and resonant Se0 photoionization cross section se1_px.dat 78 346274 Direct and resonant Se+ photoionization cross section se2_px.dat 78 358941 Direct and resonant Se2+ photoionization cross section se3_px.dat 78 164862 Direct and resonant Se3+ photoionization cross section se4_px.dat 78 74055 Direct and resonant Se4+ photoionization cross section se5_px.dat 78 98750 Direct and resonant Se5+ photoionization cross section adf/* . 12 Total and partial final state resolved dielectronic recombination rate coefficients for six ions of Se, in the ADAS adf09 and adf48 formats -------------------------------------------------------------------------------- Byte-by-byte Description of file: table1.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 4 A4 --- Ion Ion designation 6- 11 A6 --- Set Configuration set (Small, Medium or Large) 13- 15 I3 --- Nlev Number of levels 16 A1 --- n_Nlev [b] Note (1) 18-223 A206 --- Conf Configurations -------------------------------------------------------------------------------- Note (1): b: Although the same CI expansion was utilized for the small and medium sets of Se6+, the scaling parameters of the medium set were optimized differently: the configurations 3d95d, 3d96d, and 3d97d were included in the configuration list to determine scaling parameters, but removed in the final structure calculation. -------------------------------------------------------------------------------- Byte-by-byte Description of file (#): *xd.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 16 E14.8 Ry EP [0/100] Photon energy 21- 30 E10.4 Mbarn Xint Photoionization cross section (in 10-18cm2) -------------------------------------------------------------------------------- Byte-by-byte Description of file (#): *x.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 3- 16 E14.8 Ry EP Photon energy relative to the ground state 19- 32 E14.8 Ry E(N0) Photon energy relative to the initial state (1) 34- 48 E15.8 Ry E0 Ejected electron energy relative to the ground state 50- 64 E15.8 Ry E Ejected electron energy relative to the initial state 69- 78 E10.4 Mbarn Xint Photoionization cross section (in 10-18cm2) -------------------------------------------------------------------------------- Note (1): E(N0)=EP for the ground state. -------------------------------------------------------------------------------- Acknowledgements: N. Sterling, sterling(at)pa.msu.edu
(End) Patricia Vannier [CDS] 28-Feb-2011
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