The O I] 1641 Å line as a probe of symbiotic star winds

Astronomy and Astrophysics

Volumn 515, Issue 11, 2010, Pages

  Shore, S N ^a,b   Wahlgren, G M ^c,d  

^a UNIVERSITY OF PISA   (Italy)

^b INFN SEZIONE DI PISA   (Italy)

^c CATHOLIC UNIVERSITY OF AMERICA   (United States)

^d NASA GODDARD SPACE FLIGHT CENTER   (United States)

Author keywords

Atomic processes; Binaries: symbiotic; Circumstellar matter; Galaxies: active

Indexed keywords

GALAXIES; OXYGEN;

ACTIVE GALACTIC NUCLEI; ATOMIC PROCESS; BINARIES: SYMBIOTIC; CIRCUMSTELLAR MATTERS; COLUMN DENSITY; GALAXIES : ACTIVE; H II REGIONS; HIGH RESOLUTION; META-STABLE STATE; NEUTRAL MEDIUM; NEUTRAL RED; OPTICAL DEPTH; OPTICAL LIGHT; SYMBIOTIC STARS;

STARS;

EID: 77953625023     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014271     Document Type: Article

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