Journalartikel

Dielectronic recombination in photoionized gas: The importance of fine-structure core excitations


AutorenlisteSavin, DW; Bartsch, T; Chen, MH; Kahn, SM; Liedahl, DA; Linkemann, J; Müller, A; Schippers, S; Schmitt, M; Schwalm, D; Wolf, A

Jahr der Veröffentlichung1997

SeitenL115-L118

ZeitschriftThe Astrophysical Journal

Bandnummer489

Heftnummer1

ISSN0004-637X

Open Access StatusGreen

DOI Linkhttps://doi.org/10.1086/310966

VerlagAmerican Astronomical Society


Abstract
At the low electron temperatures existing in photoionized gases with cosmic abundances, dielectronic recombination (DR) proceeds primarily via nl(j) --> nl(j)' excitations of core electrons (Delta n = 0 DR). At these temperatures, the dominant DR channel often involves 2p(1/2) --> 2p(3/2) fine-structure core excitations, which are not included in LS-coupling calculations or the Burgess formula. Using the heavy-ion storage ring at the Max-Planck-Institut fur Kernphysik in Heidelberg, Germany, we have verified experimentally for Fe XVIII that DR proceeding via this channel can be significant in relation to other recombination rates, especially at the low temperatures characteristic of photoionized gases. At temperatures in photoionized gases near where Fe XVIII peaks in fractional abundance, our measured Fe XVIII to Fe XVII Delta n = 0 DR rate coefficient is a factor of similar to 2 larger than predicted by existing theoretical calculations. We provide a fit to our measured rate coefficient for ionization equilibrium models. We have carried out new fully relativistic calculations using intermediate coupling, which include the 2p(1/2) --> 2p(3/2) channel and agree to within similar to 30% with our measurements. DR via the 2p(1/2) --> 2p(1/2) channel may also have spectroscopic implications, providing unique spectral signatures at soft X-ray wavelengths that could provide good electron temperature diagnostics.



Zitierstile

Harvard-ZitierstilSavin, D., Bartsch, T., Chen, M., Kahn, S., Liedahl, D., Linkemann, J., et al. (1997) Dielectronic recombination in photoionized gas: The importance of fine-structure core excitations, The Astrophysical Journal, 489(1), pp. L115-L118. https://doi.org/10.1086/310966

APA-ZitierstilSavin, D., Bartsch, T., Chen, M., Kahn, S., Liedahl, D., Linkemann, J., Müller, A., Schippers, S., Schmitt, M., Schwalm, D., & Wolf, A. (1997). Dielectronic recombination in photoionized gas: The importance of fine-structure core excitations. The Astrophysical Journal. 489(1), L115-L118. https://doi.org/10.1086/310966



Schlagwörter


ATOMIC DATAatomic processesCOEFFICIENTSFLUORINELIKE IONSHIGH-RESOLUTION MEASUREMENTIONIZATION EQUILIBRIUMLINE EMISSIONline, formationLOW-TEMPERATURESNEONX-rays, general


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