Properties and nature of Be stars: 27. Orbital and recent long-term variations of the Pleiades Be star Pleione = BU Tauri

Astronomy and Astrophysics

Volumn 516, Issue 25, 2010, Pages

  Nemravova J ^a   Harmanec, P ^a   Kubat J ^b   Koubsky P ^b   Iliev, L ^c   Yang, S ^d   Ribeiro, J ^e   Slechta M ^b   Kotkova L ^b   Wolf, M ^a   Skoda P ^b  

^a CHARLES UNIVERSITY   (Czech Republic)

^b ASTRONOMICAL INSTITUTE   (Czech Republic)

^c INSTITUTE OF ASTRONOMY   (Bulgaria)

^d UNIVERSITY OF VICTORIA   (Canada)

^e Observatorio Do Instituto Geografico Do Exercito   (Portugal)

Author keywords

binaries: close; stars: early type; stars: emission line, Be; stars: individual: BU Tau

Indexed keywords

ELECTRON ENERGY LEVELS;

ANGULAR SEPARATION; BE STARS; BINARIES: CLOSE; CIRCUMSTELLAR MATTERS; DATA COVER; LONG-TERM CHANGES; LONG-TERM VARIATIONS; OPTICAL INTERFEROMETER; STARS: EARLY-TYPE; STARS: EMISSION-LINE , BE; STARS: INDIVIDUAL: BU TAU; TIME CHANGE; VELOCITY VARIATIONS; STARS: EMISSION-LINE, BE;

STARS;

EID: 77957590647     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/200913885     Document Type: Article

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