The O IV and S IV intercombination lines in the ultraviolet spectra of astrophysical sources

Monthly Notices of the Royal Astronomical Society

Volumn 337, Issue 3, 2002, Pages 901-909

  Keenan, F P ^a   Ahmed, S ^a   Brage, T ^b   Doyle, J G ^c   Espey, B R ^d,e   Exter, K M ^a   Hibbert, A ^a   Keenan, M T C ^f   Madjarska, M S ^c   Mathioudakis, M ^a   Pollacco, D L ^a  

^a QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

^b LUND UNIVERSITY   (Sweden)

^c ARMAGH OBSERVATORY   (United Kingdom)

^d TRINITY COLLEGE DUBLIN   (Ireland)

^e DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^f Hazelwood College   (United Kingdom)

Author keywords

Atomic data; Binaries: symbiotic; Sun: UV radiation

Indexed keywords

ASTROPHYSICS; IONIZATION POTENTIAL;

ASTROPHYSICAL SOURCES; ATOMIC DATA; BINARIES: SYMBIOTIC; INTER-COMBINATION LINE; LINE RATIOS; OBSERVATIONAL DATA; SUN:UV RADIATION; SYMBIOTIC STARS; ULTRA-VIOLET SPECTRUMS; ULTRAVIOLET SPECTRUM;

ULTRAVIOLET SPECTROSCOPY;

EID: 19044398824     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2002.05988.x     Document Type: Article

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