Constarium
← Search

Table · dataset · 2015

MgV lines collision rates for electron excitation

Listed in IVOA Registry (Virtual Observatory)

Transition probabilities and electron impact excitation collision strengths and rates for astrophysically important lines in Mg V are reported.

Description

The 86 fine-structure levels of the 2s^2^2p^4^, 2s2p^5^, 2p^6^, 2s2^2^p^3^3s, 2s^2^2p^3^3p and 2s^2^2p^3^3d configurations are included in our calculations. The effective collision strengths are presented as a function of electron temperature for solar and other astrophysical applications.

Links

Where it is published

Documentation and papers

Catalogue records · 2

Topics

Provenance · 1 source records, 7 field assertions
SourceKeyLast seenRaw
IVOA Registry (Virtual Observatory)ivo://cds.vizier/j/a+a/574/a8712 d agoJSON v1
FieldAssertionExtractorEvidence
access_levelsource · IVOA Registryconnector:ivoa_registry@1.0.0
concepts[field].local:field:astronomymapping · IVOA Registryconnector:ivoa_registry@1.0.0
descriptionsource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_description
license_textsource · IVOA Registryconnector:ivoa_registry@1.0.0
publication_datesource · IVOA Registryconnector:ivoa_registry@1.0.0
titlesource · IVOA Registryconnector:ivoa_registry@1.0.0rr.resource.res_title
updated_datesource · IVOA Registryconnector:ivoa_registry@1.0.0