OVI in the local interstellar medium: FUSE observations towards B-stars within 200 pc

Astronomy and Astrophysics

Volumn 490, Issue 2, 2008, Pages 707-714

  Welsh, B Y ^a   Lallement, R ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b CNRS   (France)

Author keywords

Galaxy: solar neighborhood; ISM: atoms; Ultraviolet: ISM

Indexed keywords

ABSORPTION; ABSORPTION SPECTROSCOPY; CHARGE TRANSFER; CURVE FITTING; GAS ABSORPTION; GAS FUEL PURIFICATION; GASES; NASA; SIZE DISTRIBUTION; SOLAR WIND; STARS;

ABSORPTION LINES; ABSORPTION MODELS; BACKGROUND SIGNALS; CENTRAL REGIONS; COLUMN DENSITIES; CONDUCTIVE; CURRENT THEORETICAL MODELS; EQUIVALENT WIDTHS; FAR ULTRAVIOLETS; GALACTIC LATITUDES; GALACTIC PLANES; GALAXY: SOLAR NEIGHBORHOOD; ISM: ATOMS; LINE PROFILES; LOCAL INTERSTELLAR MEDIUMS; SOLAR WIND CHARGE EXCHANGES; SPATIAL DISTRIBUTION OF; SPECTRAL DATUM; SPECTROSCOPIC OBSERVATIONS; TRANSITION LAYERS; ULTRAVIOLET: ISM; UPPER LIMITS;

PHASE INTERFACES;

EID: 54549093823     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361:200810221     Document Type: Article

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