RECOMBINATION COEFFICIENTS FOR O-II LINES AT NEBULAR TEMPERATURES ANDDENSITIES

Authors
STOREY PJ
Citation
Pj. Storey, RECOMBINATION COEFFICIENTS FOR O-II LINES AT NEBULAR TEMPERATURES ANDDENSITIES, Astronomy and astrophysics, 282(3), 1994, pp. 999-1013
Citations number
23
Categorie Soggetti
Astronomy & Astrophysics
Journal title
Astronomy and astrophysics → ACNP
ISSN journal
00046361
Volume
282
Issue
3
Year of publication
1994
Pages
999 - 1013
Database
ISI
SICI code
0004-6361(1994)282:3<999:RCFOLA>2.0.ZU;2-F
Abstract
Rate coefficients are calculated for the formation of O(II) lines by r ecombination. Photoionization data from the Opacity Project are used t o calculate recombination coefficients for principal quantum numbers, n less-than-or-equal-to 10, including radiative and dielectronic recom bination. Cascading from higher states is included, allowing for the e ffects of finite electron density in a hydrogenic approximation.