The pulsation of χ cygni imaged by optical interferometry: A novel technique to derive distance and mass of mira stars

Astrophysical Journal

Volumn 707, Issue 1, 2009, Pages 632-643

  Lacour, S ^a   Thiebaut E ^b   Perrin, G ^a   Meimon, S ^c   Haubois, X ^a   Pedretti, E ^d   Ridgway, S T ^e   Monnier, J D ^f   Berger, J P ^g   Schuller, P A ^h   Woodruff, H ⁱ   Poncelet, A ^a   Le Coroller, H ^j   Millan Gabet, R ^k   Lacasse, M ^l   Traub, W ^m  

^a UNIVERSITÉ PARIS DIDEROT   (France)

^b CENTRE DE RECHERCHE ASTROPHYSIQUE DE LYON   (France)

^c Office National d'Etudes et de Recherches Aerospatiales   (France)

^d UNIVERSITY OF ST ANDREWS   (United Kingdom)

^e NATIONAL OPTICAL ASTRONOMY OBSERVATORY   (United States)

^f UNIVERSITY OF MICHIGAN   (United States)

^g CNRS   (France)

^h UNIVERSITÉ PARIS SUD   (France)

ⁱ UNIVERSITY OF SYDNEY   (Australia)

^j OBSERVATOIRE DE HAUTE PROVENCE   (France)

^k CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^l HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^m CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

more..

Author keywords

Infrared: stars; Stars: AGB and post AGB; Stars: fundamental parameters; Stars: individual (chi Cyg); Techniques: interferometric

Indexed keywords

EID: 72849135957     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1088/0004-637X/707/1/632     Document Type: Article

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