Lines of O IV and S IV in the Goddard high-resolution spectrograph spectrum of RR Tel: Constraints on atomic data

Monthly Notices of the Royal Astronomical Society

Volumn 303, Issue 3, 1999, Pages

  Harper, G M ^a   Jordan, C ^b   Judge, P G ^c   Robinson, R D ^d   Carpenter, K G ^e   Brage, T ^f  

^a UNIVERSITY OF COLORADO   (United States)

^b UNIVERSITY OF OXFORD   (United Kingdom)

^c NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^d CATHOLIC UNIVERSITY OF AMERICA   (United States)

^e NASA GODDARD SPACE FLIGHT CENTER   (United States)

^f LUND UNIVERSITY   (Sweden)

Author keywords

Atomic data; Binaries: symbiotic; Stars: individual: RR Tel; Ultraviolet: stars

Indexed keywords

ATOMS; SIGNAL TO NOISE RATIO; STARS;

ATOMIC DATA; BINARIES: SYMBIOTIC; FLUX RATIO; HIGH RESOLUTION; HIGH SIGNAL-TO-NOISE RATIO; RATIO SPECTRA; SPECTRA'S; STAR: INDIVIDUAL: RR TEL; STARS: INDIVIDUAL: PROXIMA CENTAURI; ULTRAVIOLET: STARS;

SPECTROGRAPHS;

EID: 0002477318     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1999.02392.x     Document Type: Article

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