HD 108: The mystery deepens with XMM-Newton observations

Astronomy and Astrophysics

Volumn 417, Issue 2, 2004, Pages 667-677

  Naze Y ^a,b   Rauw, G ^a,b   Vreux, J M ^a   De Becker, M ^a  

^a UNIVERSITY OF LIÈGE   (Belgium)

^b FNRS   (Belgium)

Author keywords

Stars: early type; Stars: individual: HD 108; Stars: winds, outflows; X rays: stars

Indexed keywords

APPROXIMATION THEORY; HARDNESS; JETS; LIGHT ABSORPTION; LIGHT EMISSION; PLASMAS; SENSITIVITY ANALYSIS; SPECTROSCOPIC ANALYSIS; WIND; X RAY ANALYSIS;

STARS: EARLY-TYPE; STARS: INDIVIDUAL: HD 108; STARS: OUTFLOWS; STARS: WINDS; X-RAYS: STARS;

ASTRONOMY;

EID: 1842739081     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20034422     Document Type: Article

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