The He II Fowler lines and the O III and N III Bowen fluorescence lines in the symbiotic nova RR Telescopii

Astronomy and Astrophysics

Volumn 464, Issue 2, 2007, Pages 715-734

  Selvelli, P ^a   Danziger, J ^a   Bonifacio, P ^a,b,c  

^a INAF OSSERVATORIO ASTRONOMICO DI TRIESTE   (Italy)

^b CIFIST Marie Curie Excellence Team ^*

^c OBSERVATOIRE DE PARIS   (France)

Author keywords

Atomic processes; Radiative transfer; Stars: binaries: symbiotic; Stars: novae, cataclysmic variables; Ultraviolet: stars

Indexed keywords

FLUORESCENCE; LIGHT EMISSION; LIGHT SCATTERING; RADIATIVE TRANSFER; SPACE RESEARCH; TELESCOPES;

ATOMIC PROCESSES; BOWEN MECHANISM; CONTINUUM DISTRIBUTION; CONTINUUM FLUORESCENCE;

STARS;

EID: 33947228388     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:20066175     Document Type: Article

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