Time-resolved high-resolution spectroscopy of CH Cygni: Evidence for a magnetic propeller state in 1994

Monthly Notices of the Royal Astronomical Society

Volumn 278, Issue 2, 1996, Pages 542-550

  Tomov, T ^a   Kolev, D ^a   Munari, U ^b   Antov, A ^c  

^a National Astronomical Observatory Rozhen   (Bulgaria)

^b Osservatorio Astronomico di Padova   (Italy)

^c Astronomical Observatory   (Bulgaria)

Author keywords

Binaries: symbiotic; Line: profiles; Stars: individual: CH Cyg

Indexed keywords

FIGHTER AIRCRAFT; PROPELLERS; STARS;

BINARIES: SYMBIOTIC; HIGH RESOLUTION; HIGH-RESOLUTION SPECTROSCOPY; LINE: PROFILES; RESOLUTION TIME; SPATIALLY RESOLVED; STAR: INDIVIDUAL: CH CYG; STARS: INDIVIDUAL: PROXIMA CENTAURI; TIME-RESOLUTION; TIME-RESOLVED;

SPECTROSCOPIC ANALYSIS;

EID: 0002072062     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/278.2.542     Document Type: Article

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