Imaging the asymmetric dust shell around CI Cam with long baseline optical interferometry

Monthly Notices of the Royal Astronomical Society

Volumn 398, Issue 3, 2009, Pages 1309-1316

  Thureau, N D ^a   Monnier, J D ^b   Traub, W A ^c   Millan Gabet, R ^d   Pedretti, E ^a   Berger, J P ^e   Garcia, M R ^f   Schloerb, F P ^g   Tannirkulam, A K ^b  

^a UNIVERSITY OF ST ANDREWS   (United Kingdom)

^b UNIVERSITY OF MICHIGAN   (United States)

^c CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e LABORATOIRE D ASTROPHYSIQUE   (France)

^f HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^g UNIVERSITY OF MASSACHUSETTS   (United States)

Author keywords

Circumstellar matter; Stars: individual: CI Cam; Techniques: High angular resolution; Techniques: interferometric

Indexed keywords

CAMS; INFRARED DEVICES; INTERFEROMETRY; STARS; TELESCOPES; VISIBILITY;

CIRCUMSTELLAR; CIRCUMSTELLAR MATTERS; CLOSURE PHASE; LONG BASE LINE; NEAR INFRARED; NEAR-INFRARED; STAR: INDIVIDUAL: CI CAM; STARS: INDIVIDUAL: PROXIMA CENTAURI; TECHNIQUE: INTERFEROMETRIC; TECHNIQUES: HIGH ANGULAR RESOLUTIONS;

DUST;

EID: 70249100273     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14949.x     Document Type: Article

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