UCL logo

UCL Discovery

UCL home » Library Services » Electronic resources » UCL Discovery

RECOMBINATION COEFFICIENTS FOR O-II LINES AT NEBULAR TEMPERATURES AND DENSITIES

STOREY, PJ; (1994) RECOMBINATION COEFFICIENTS FOR O-II LINES AT NEBULAR TEMPERATURES AND DENSITIES. ASTRON ASTROPHYS , 282 (3) 999 - 1013.

Full text not available from this repository.

Abstract

Rate coefficients are calculated for the formation of O(II) lines by recombination. Photoionization data from the Opacity Project are used to calculate recombination coefficients for principal quantum numbers, n less-than-or-equal-to 10, including radiative and dielectronic recombination. Cascading from higher states is included, allowing for the effects of finite electron density in a hydrogenic approximation.

Type: Article
Title: RECOMBINATION COEFFICIENTS FOR O-II LINES AT NEBULAR TEMPERATURES AND DENSITIES
Keywords: ATOMIC DATA, H-II REGIONS, PLANETARY NEBULAE, GENERAL, DIELECTRONIC RECOMBINATION, OPACITY CALCULATIONS, HYDROGENIC IONS, ATOMIC DATA, INTENSITIES
UCL classification: UCL > School of BEAMS > Faculty of Maths and Physical Sciences > Physics and Astronomy
URI: http://discovery.ucl.ac.uk/id/eprint/99000
Downloads since deposit
0Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item