Energy levels, radiative rates, and electron impact excitation rates for transitions in OVII


Autoria(s): Aggarwal, K. M.; Keenan, F. P.
Data(s)

01/10/2008

Resumo

Aims. <br/>In this paper we report calculations for energy levels, radiative rates, and electron impact excitation rates for transitions in O vii.<br/>Methods. <br/>The grasp (general-purpose relativistic atomic structure package) is adopted for calculating energy levels and radiative<br/>rates. For determining the collision strengths and subsequently the excitation rates, the Dirac atomic R-matrix code (darc) and the<br/>flexible atomic code (fac) are used.<br/>Results. <br/>Oscillator strengths, radiative rates, and line strengths are reported for all E1, E2, M1, and M2 transitions among the lowest<br/>49 levels of O vii. Collision strengths have been averaged over a Maxwellian velocity distribution, and the resulting effective collision<br/>strengths are reported over a wide temperature range below 2 × 106 K. Additionally, lifetimes are also listed for all levels.<br/>Key words.

Formato

application/pdf

Identificador

http://pure.qub.ac.uk/portal/en/publications/energy-levels-radiative-rates-and-electron-impact-excitation-rates-for-transitions-in-ovii(3ff888ef-d801-4dca-86b5-040b5ad9307a).html

http://dx.doi.org/10.1051/0004-6361:200810531

http://pure.qub.ac.uk/ws/files/16339825/aa10531_08.pdf

Idioma(s)

eng

Direitos

info:eu-repo/semantics/openAccess

Fonte

Aggarwal , K M & Keenan , F P 2008 , ' Energy levels, radiative rates, and electron impact excitation rates for transitions in OVII ' Astronomy and Astrophysics , vol 489 , pp. 1377-1388 . DOI: 10.1051/0004-6361:200810531

Palavras-Chave #/dk/atira/pure/subjectarea/asjc/1900/1912 #Space and Planetary Science #/dk/atira/pure/subjectarea/asjc/3100/3103 #Astronomy and Astrophysics
Tipo

article