Energy levels, radiative rates, and electron impact excitation rates for transitions in OVII
Data(s) |
01/10/2008
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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 | |
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 |