Dielectronic Recombination in Photoionized Gas: The Importance of Fine-structure Core Excitations | Zendy

D. W. Savin | Zendy; Thomas Bartsch | Zendy; M. H. Chen | Zendy; S. M. Kahn | Zendy; D. A. Liedahl | Zendy; J. Linkemann | Zendy; A. Müller | Zendy; S. Schippers | Zendy; M. Schmitt | Zendy; D. Schwalm | Zendy; A. Wolf | Zendy

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Dielectronic Recombination in Photoionized Gas: The Importance of Fine-structure Core Excitations

Author(s) -

D. W. Savin,

Thomas Bartsch,

M. H. Chen,

S. M. Kahn,

D. A. Liedahl,

J. Linkemann,

A. Müller,

S. Schippers,

M. Schmitt,

D. Schwalm,

A. Wolf

Publication year - 1997

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/310966

Subject(s) - physics , ionization , atomic physics , recombination , ion , electron , core (optical fiber) , coupling (piping) , astrophysics , nuclear physics , optics , biochemistry , chemistry , gene , mechanical engineering , quantum mechanics , engineering

At the low electron temperatures existing in photoionized gases with cosmic abundances, dielectronic recom- bination (DR) proceeds primarily via excitations of core electrons ( DR). At these temperatures, 0 nl r nl Dn 5 0 0 jj the dominant DR channel often involves

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